Constellation Cygnus (Swan)

Cygnus
Cygnus: IAU Constellation Map [150]

Properties

Cygnus is a very showy and beautiful summer constellation. Its brightest stars form a figure that one can associate with the corresponding shape of the swan without much imagination. The tail of the swan sailing across the Milky Way is marked by Deneb, its head by Albireo and the two wings by delta and epsilon Cygni. Cygnus lies in a star-rich region of the Milky Way, which appears to be divided into two parts by an extensive dark cloud on dark nights. Deneb, the main star, is a corner point of the famous summer triangle, which is completed by Atair and Wega. The constellation Cygnus extends over an area of 804 square degrees in the sky and the center culminates around midnight on July 29th. [9, 15]

Stars with Proper Names:

  • α Cyg: Deneb, Deneb Cygni, Deneb El Adige, Arided, Aridif, Gallina, Arrioph
  • β1 Cyg: Albireo
  • γ Cyg: Sadr, Sador, Sadir
  • ε Cyg: Gienah Cygni, Gienah
  • π1 Cyg: Azelfafage
Data for constellation Cygnus [150]
IAU NameCygnus
IAU GenitiveCygni
IAU Abbr.Cyg
English NameSwan
Season (47° N)March … December
Right Ascension19h 07m 30s … 22h 03m 03s
Declination+27° 43' 57" … +61° 21' 28"
Area804 deg2
Neighbours (N↻)Cep, Dra, Lyr, Vul, Peg, Lac

Deep-Sky Object Descriptions

Constellation Cygnus
Constellation Cygnus: Illustration from «Uranometria» by Johann Bayer, copper engraving by Alexander Mair, 1603 [28]

Mythology and History

In Greek mythology, Cyknos (Cygnus) was a musician king and a devoted friend of Phaethon, the son of the sun god Helios. One day Phaethon persuaded his father to let him lead the sun chariot across the sky, but then he lost control of the horses and wreaked havoc on heaven and earth. The king of the gods, Zeus, hurled one of his thunderbolts at Phaethon, killing him instantly. His still smoldering body fell into the river Eridanus. Kyknos jumped into the river, swam back and forth and kept diving to find his friend's body. It was said that it looked like a swan swimming in the water, diving for food. Helios looked on sadly and picked up his son's loyal friend and sat him on a place between the stars in the firmament. [71]

Cygnus
Cygnus: Milky Way with dark clouds and bright nebulae; Nikon D3, Nikkor 24-70mm 2.8G @ f/4, SkyWatcher StarAdventurer Pro; L: 50*120s, D: 15*120s, F: 15, ISO 1600; Glaubenberg Pass; © 18. 9. 2020 Bernd Nies

In another version of this myth, Cygnus wandered in a poplar grove on the bank of the Eridanus River, mourning the death of his friend. In the end, the gods pitied him so much that they turned him into a swan of stars. Since then it has been said that swans sang sad songs when they are about to die. This is the origin of the expression "swan song", which denotes the last work of a musician or poet before his death. [71]

At another time and place in Greek mythology, Zeus slipped into the shape of a swan in order to be able to approach Leda, the wife of King Tyndareus of Sparta, who was bathing her lovely body in the river. The immortal children of Leda, who had Zeus for their father, were Helena and Pollux. The mortal children she bore to her husband Tyndareus were Castor and Clytemnestra. [7, 20]

In Arabia, the constellation has been seen as a flying bird. In Christian symbolism it was interpreted as the crux of Christ, the cross on Calvary and the northern cross. [20, 54]

Catalogs

Yale Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991) [154]
HR B F DM HD SAO FK5 IR M* ADS VarID RA Dec vMag spType dMag Sep ["] Remarks
HR 7275BD+52 235017909431413I V1762 Cyg19 08 25.8+52 25 325.81 K1IV SB:28.59d, K 40.3k/s, V0 +5.2k/s, asini 15.8.,VAR:Amp. 0.05V.
HR 7293BD+49 29591799574819212169 B19 12 04.6+49 51 156.75 G4V 0.28.1D:Binary with HR 7294. C, 12.7v at 56" optical.,DYN:0.058".
HR 7294BD+49 29591799584819312169 A19 12 05.0+49 51 226.57 G4V 0.28.1D:See HR 7293.,DYN:0.058".
HR 7311BD+49 29681807564824712240 19 15 19.3+50 04 156.27 R G8III 4.52.1D:AB, CPM.
HR 7322BD+46 2658181096482783541 19 16 51.4+46 59 576.00 F6IV:
HR 7328κ1BD+53 221618127631537726I 1188619 17 06.2+53 22 073.77 G9III VAR:SRd?, 3.76 - 3.82V, 79d?
HR 7341BD+49 297718159748315 19 18 37.7+49 34 116.31 K1III vVAR:Spectrum var. 8.115813d.
HR 7351BD+54 212318196031574 19 19 36.5+54 22 346.26 A1V
HR 73722BD+29 3584182568871593550W 19 24 07.6+29 37 174.97 B3IV
HR 7374BD+27 337918261887165 19 24 22.4+28 05 166.53 B5V
HR 7381BD+49 2994182691316233549 19 23 23.8+50 16 176.51 B9III
HR 73954BD+36 3557183056683013554 V1741 Cyg19 26 09.1+36 19 045.15 B9pSi S:Magnetic star.,SB:35.0225d, K 5.7k/s, V0 -11.0k/s, asini 2.45.,VAR:Alpha CV, amp. 0.02U, 0.68674d.
HR 7408ι17BD+52 243418353431673 19 27 25.9+52 19 145.75 A1V
HR 7417β16BD+27 341018391287301732I12540 A1210519 30 43.3+27 57 353.08 K3II+B9.5V 2.034.7D:7270.2y, a = 62.90". Binary with HR 7418. vsini of B-type component of ADS 12540A 50:k/s. Component C, 11v at 50".,D:Two additional components of A resolved by speckle interferometry: Aa 1981.70, sep. 0.42"; Ap 1978.41, sep. 0.12" and,D:1979.46, sep. <0.08".,DYN:0.009".,N:ALBIREO.
HR 7418β26BD+27 34111839148730212540 B19 30 45.3+27 57 555.11 B8Ve 2.034.7D:See HR 7417. Unresolved by speckle interferometry 1981.47, sep. <0.03".,DYN:0.009".
HR 7419BD+35 36581839866841712545 19 30 46.9+36 13 436.25 B9.5III 7.727.7
HR 7420ι210BD+51 260518400631702733 19 29 42.3+51 43 473.79 A5Vn
HR 74268BD+34 3590184171684471510 19 31 46.3+34 27 114.74 B3IV
HR 7427BD+49 303418429331737I 19 31 19.3+50 18 245.53 gK1
HR 7428BD+55 221518439831741 V1817 Cyg19 31 13.6+55 43 556.37 K2II-IIIe+A0V vS:Strong CaII emission.,SB:108.5707d, K 22.1k/s, V0 -5.2k/s, asini 33.0. vsini of both components =<50k/s.,VAR:RS CVn. Amp. about 0.045V, 108.5707d. Variable H alpha emission.
HR 7436BD+38 365018460368499S 19 33 36.4+38 45 446.61 A3Vn 0.1
HR 74419BD+29 365118475987385W 19 34 50.9+29 27 475.38 F8III+A0V 0.50.1D:Visual companion CPM.,S:Also classified F5V + A and gG + late A.,SB:1717.3d, K 15.7k/s, V0 -17.1k/s, asini 261; vsini of both components =<50k/s; speckle interferometry 1985.5 gives,SB:sep. 0.053"; 1986.46, sep. 0.035" (at 7000 Ang.). Alternate orbit 215.48d, K 14.5k/s, V0 -15.8k/s, asini 40.8.,SB:Morbey and Griffin (1987, ApJ, 317, 343) reject these orbits and claim a period of about 1573d.
HR 7442BD+48 291418478648589I V1743 Cyg19 33 41.6+49 15 455.96 M4.5IIIaS VAR:SRb?, amp. 0.18V, 40:d.
HR 7444BD+42 338618487548601 19 34 41.2+42 24 465.35 A2V
HR 7451BD+50 281518496031782 19 34 19.8+51 14 125.73 F7V G:Sirius group; UMa stream.
HR 7453BD+47 287018497748606 19 34 39.9+48 09 536.67 R A9V
HR 745711BD+36 361918503768552 19 35 48.3+36 56 406.05 B8Vne S:Shell star.
HR 7465BD+49 305918526431804 19 35 55.9+50 14 196.52 G9III
HR 7466BD+29 36701852688746212696 19 37 09.4+29 20 016.43 B5V 2.720.6D:AP, sep. 0.1" unresolved by speckle interferometry at eight epochs between 1976.45 and 1981.70 (McAlister and Hartkopf).
HR 7467BD+38 367718533068585 19 36 56.6+38 23 026.50 B5II-III G:Member of the local association (Pleiades group).
HR 7468BD+44 318518535148649 19 36 37.9+44 41 425.17 G9IIIbFe-0.5
HR 7469θ13BD+49 306218539531815738I12695 19 36 26.5+50 13 164.48 F4V 6.948.4D:AB CPM. B, 13v at 3". C, optical.
HR 7477BD+48 292218565748673W 19 37 56.7+49 17 046.47 G6V 2.929.6S:Also classified G9III.
HR 7478φ12BD+29 3684185734686373570IS 19 39 22.6+30 09 124.69 G8III-IV 0.0D:1.188y, a = 0.026".,SB:434.086d, K 26.8k/s, V0 +5.0k/s, msin3i 2.35, asini 137. Resolved by speckle interferometry. Rare example of,SB:SB2 composed of 2 giants; similar spectra.
HR 7481BD+33 35471858376865412765 19 39 45.0+33 58 456.10 A3IV 4.51.3D:AB binary.
HR 748314BD+42 3413185872486913572 19 39 26.5+42 49 065.40 B9III
HR 7484BD+54 2193185912318503571 V1143 Cyg19 38 41.2+54 58 265.82 F6Va S:Also classified F5V + F5V.,SB:7.6408d, K 87.1k/s, V0 -15.9k/s, msin3i 1.33, asini 7.70.,VAR:EA 5.85 - 6.37V, 7.6407613d.
HR 7487BD+45 294018595548697 19 39 34.4+45 57 296.20 G8-K0II-III
HR 7492BD+42 341918612148714I 19 40 41.2+43 04 406.16 M2III
HR 7495BD+45 2949186155487183575W 1230019 40 50.2+45 31 305.06 F5II-III 6.788.0
HR 7499BD+39 387818630748737W 19 41 57.5+40 15 146.23 A6V 1.30.2
HR 7501BD+28 344718635787612 V1276 Cyg19 42 49.1+29 19 546.49 F1III VAR:Delta Sct 6.50 - 6.53V, 0.088d.
HR 7502BD+32 3531186377687303577 19 42 44.6+32 25 365.94 A5III
HR 750316BD+50 28471864083189812815 A19 41 48.9+50 31 315.96 G1.5Vb 0.239.2D:Binary with HR 7504. Third component mag. diff 7.17V, sep. 70" from A.,DYN:0.072".
HR 7504BD+50 28481864273189912815 B19 41 52.0+50 31 036.20 G2.5V 0.239.2D:See HR 7503.,DYN:0.072".
HR 7505BD+30 370618644068744 19 43 09.5+30 40 436.05 A1V
HR 7509BD+55 224518653231906I V1351 Cyg19 42 04.1+55 27 486.48 M5IIIa VAR:Lb 6.33 - 6.55V. B-V from +1.57 to 1.62.
HR 7512BD+33 35721865686876412852 19 43 51.4+34 09 456.05 B8III 7.333.9
HR 7514BD+41 346918661948771I 19 43 45.0+41 46 235.84 M0IIIab
HR 751715BD+37 358618667568778740I 19 44 16.6+37 21 164.89 G7+III
HR 7518BD+28 346018668887659 SU Cyg19 44 48.7+29 15 536.82 F2I vS:Also classified F0-G1II, G0III and F2-G0II-III + B7V.,VAR:CDelta 6.44 - 7.22V, 3.8455473d. Period changes.
HR 7520BD+34 369118670268783I 1237219 44 38.2+34 24 506.57 R M1III
HR 7522BD+57 205718676031923 19 43 14.6+58 00 596.22 G0V
HR 7523BD+40 386618677648789I V973 Cyg19 44 49.0+40 43 006.34 M4-III G:Arcturus group.,M:High space velocity.,VAR:SRb 7.8 - 8.6p, about 40d.
HR 7526BD+56 229118681531933 19 43 39.6+57 02 336.27 K2III
HR 7528δ18BD+44 323418688248796I12880 12380/119 44 58.5+45 07 512.87 B9.5IV+F1V 3.52.0C:Color excess E(B-V) = +0.05.,D:AB 2.91 B9.5III, 6.33 F1V, 827.6y, a = 3.20".,DYN:0.021".,VAR:ADS 12880A is NSV 12381, 2.85 - 2.89V. Component B is NSV 12380, 6.5 ->8.5v.
HR 7529BD+35 37861869016880512893 A19 45 39.6+36 05 286.43 B9.5VpSi 0.514.8D:AB binary. B is 7.16V, +0.02(B-V), -0.07(U-B), B9.5V, vsini 250k/s.,S:Silicon star?
HR 7530BD+34 37011869276881012900 19 45 51.4+35 00 466.09 K0II-III+A2V 2.444.6D:Component B, 8.56V, +0.05(B-V), +0.11(U-B), A2V at 39".
HR 753417BD+33 35871870136882712913 A1239819 46 25.6+33 43 404.99 F7V 3.526.0D:AB binary. B is dK6. Component C, optical. ADS 12913AB and ADS 12889 (9.2, 9.4 dK5 sep. 3") at 792" are CPM and have,D:same RV and parallax. ADS 12889, 259y, a = 2.27", mean mass 0.6 solar.,DYN:0.042".,VAR:ADS 12913B, 8.55 - 8.60V; difference between components varies from 1.9 to 3.3p.
HR 7535BD+32 35581870386883512920 19 46 35.0+32 53 196.18 K3III 2.130.7D:B, 13v at 3" binary with A. C, 14v at 10" binary with A. D, optical.
HR 7543BD+38 37581872356885912944 19 47 27.8+38 24 275.77 B8Vn 7.224.7
HR 7547BD+47 291618737248842I 19 47 26.8+47 54 286.12 M2III
HR 7550BD+34 37271874586889312972 19 48 43.9+35 18 416.53 F4V 0.60.6D:7.2 F5V, 7.7 F7V, 156.52y, a = 0.624" or 157.21y, a = 0.607". Combined mag., colors.,DYN:0.015".,S:Composite spectrum F6Vp: met., F2; CH, F4.
HR 7551BD+33 360218745968895 V1765 Cyg19 48 50.6+33 26 146.44 B0.5Ib G:Cyg OB5.,S:No emission in H alpha has been detected, but some lines show asymmetry with the blue wings the stronger, perhaps,S:suggestive of an expanding shell.,SB:13.37383d, K 105.3k/s, V0 +9.7k/s, asini 56.6.,VAR:6.44 - 6.50V.
HR 7555BD+38 37721876386890912992 19 49 27.5+38 42 366.11 G5-8III 4.911.6
HR 7564χBD+32 359318779668943IW Chi Cyg19 50 33.9+32 54 514.23 S6+/1e v5.2158.0S:Probable SiO maser emission. Most intense infrared CO bands observed in any star to 1973. Technetium found in,S:spectrum. Also classified S6,2e-S10,4e.,VAR:Discovered by Kirch in 1686. M 3.3 - 14.2v. Period changes: 1686-1842, 405.88d; subsequently 408.05d.,VAR:Variable CO emission from circumstellar envelope and enhancement of shell at minimum light. Total visual absorption of,VAR:shell = 2 mag. Variable SiO maser source. Appreciable reddening at ascending light.
HR 756619BD+38 378018784968947I13014 V1509 Cyg19 50 34.0+38 43 215.12 M2IIIa 6.455.5D:Component B, optical.,VAR:Lb 5.08 - 5.4v.
HR 7567BD+40 3902187879488923584 V380 Cyg19 50 37.3+40 35 595.69 B1III+B3V SB:12.4256d, K 92.7k/s, V0 -2.9k/s, msin3i 12.9, asini 15.5. Apsidal period about 1490 yrs.,VAR:EA 5.61 - 5.78V, 12.42612d. Period changes.
HR 7568BD+37 363618788068953I 19 50 47.0+37 49 356.06 M4IIb
HR 757620BD+52 2547188056320423586I 1248119 50 37.7+52 59 175.03 K3IIICN1 VAR:I 6.4 - 6.52p.
HR 7577BD+47 293718807448907 Var?19 51 19.4+47 22 386.20 F2V VAR:Variability suspected on basis of comparison stars, both of which are either variable or suspected of variability.
HR 7583BD+36 374418814969004I 19 52 16.3+36 25 566.10 K4III
HR 7589BD+46 2793188209489173588 Var19 51 59.1+47 01 395.62 O9.5Ia S:Also classified O9.5Iab.,VAR:Amp. 0.05B.
HR 7591BD+47 293918825248920 1251119 52 07.2+47 55 555.91 B2III
HR 7600BD+47 294518843948940 V819 Cyg19 53 01.2+47 48 276.29 B0.5IIIn M:Old disk population runaway star.,VAR:Beta C? 6.26 - 6.30V, 0.3775d.
HR 7606BD+36 376618865069072 19 54 48.3+36 59 465.76 G1Ib-IICH1Fe-1Ca-1 S:Enhanced CH and lithium.
HR 7607BD+29 38021886516907913117 19 55 06.5+30 11 436.57 B6V+A5V 2.99.3
HR 760823BD+57 208418866532085 19 53 17.4+57 31 255.14 B5V G:Member of the local association (Pleiades group).
HR 7611BD+59 213718879332093W 19 53 35.4+59 42 326.06 A3V 3.371.4
HR 761322BD+38 381718889269101 19 55 51.7+38 29 124.94 B5IV G:Member of the local association (Pleiades group).
HR 7615η21BD+34 3798188947691161521I13149 1258619 56 18.4+35 05 003.89 K0III 7.746.0D:AB CPM. B, 12v at 7". Other components optical.,DYN:0.035".
HR 7619ψ24BD+52 25721890373211413148 19 55 37.8+52 26 204.92 A4Vn 2.33.1D:AB combined mag., colors. Sources differ on spectral class of component B from A7V to F4V. vsini of B, 120k/s.,DYN:0.008".
HR 7620BD+35 387818906669129 19 56 44.2+36 15 036.02 B5IV G:Member of the local association (Pleiades group).
HR 7626BD+57 209218912732116 19 55 22.1+58 15 016.09 G9III
HR 7628BD+39 3968189178490113593W 19 57 13.9+40 22 055.45 B5V 3.064.6G:Member of the local association (Pleiades group).,SB:71.80d.
HR 7632BD+50 293018925332130 19 56 45.1+50 54 096.43 A1V
HR 7633BD+58 2013189276321223591I 19 55 55.4+58 50 464.96 K5II-III
HR 7634BD+56 233118929632128 19 56 19.0+56 41 136.12 R A4Vn
HR 7638BD+41 35491893774903113186 19 57 56.2+42 15 396.43 R A3V 1.20.1D:AB and AC binary. C, 9.0v Am(A2/A8/A8) at 3", physical.,SB:ADS 13186A.
HR 7640BD+30 3837189395691883594 19 58 38.0+30 59 015.49 B9Vn
HR 7642BD+37 37031894326919313198 19 58 34.4+38 06 206.32 B5IV 1.11.9
HR 7646BD+45 302518968449058 19 59 20.5+45 46 205.92 A5III
HR 764725BD+36 3806189687692313599 V1746 Cyg19 59 55.2+37 02 345.19 B3IVe SB:80.0d. vsini 230k/s.,VAR:Gamma Cas + Beta Cep, amp. 0.07V, 0.20:d.
HR 7651BD+51 272818977532170 19 59 15.4+52 03 216.15 B5III
HR 7655BD+36 382018994269267 20 01 15.3+37 05 566.20 K0III
HR 766026BD+49 315819014749098I13278 A20 01 21.6+50 06 175.05 K1II-III 3.841.8
HR 7670BD+29 387219036088133 20 03 37.4+29 53 485.71 G6IV+M6V 9.8179. D:Companion 16.4pgM6, CPM.,S:Iron-rich star.
HR 7678BD+31 39251906036936213335 V1768 Cyg20 04 36.1+32 13 075.64 B1.5Ia e4.532.1D:Optical companion, +0.74(B-V), +0.34(U-B).,G:Vul OB2; in reflection nebula; member assoc. Cyg R1 at 1000 pc.,S:Shell star.,VAR:Amp. 0.08B, about 26d. Mass loss 0.00005 solar masses/y.
HR 7683BD+38 38961907716937713348 20 05 09.8+38 28 426.19 G5IV 6.140. D:B, 13.2v at 12", optical. C, 12.5v at 40".
HR 7684BD+47 3004190781491523610S 20 04 28.8+48 13 476.16 A2IV 0.3
HR 7687BD+51 276319096432272I 20 05 06.7+51 50 226.14 M1IIIa
HR 768927BD+35 395919102669413W Var?20 06 21.8+35 58 215.36 K0IV 4.011.9D:AD CPM. B, 13.7v at 23"; C, 11.6v at 36".,VAR:5.36 - 5.41V.
HR 7692BD+55 232419109632276 20 05 21.5+56 20 296.21 F4V
HR 7697BD+52 2623191195322863613W 20 06 13.8+53 09 575.85 F5V 3.8170.4
HR 7699BD+34 3881191243694573615 20 07 41.4+34 25 236.11 B5Ib G:Cyg OB3.
HR 7702BD+49 319519132932296 20 07 11.5+50 13 456.54 A3V
HR 770828BD+36 3907191610695181525 V1624 Cyg20 09 25.6+36 50 234.93 B2.5Ve vS:In 1957 B type changed to Be.,SB:226.0d. Also RV periods 45.33 and 1.51775d.,VAR:SX Ari 4.91 - 4.97V, 0.07d. Possibly also Gamma Cas type. H-line widths vary in cycles about 15 yrs.
HR 7721BD+47 304519227649314 20 12 03.8+47 44 136.92 B7V SB:7.18584d, K 18.5k/s, V0 -21.6k/s. Possibly third component.
HR 7726BD+51 27961924393235413535 20 12 31.8+51 27 496.01 K2.5III 5.64.0D:AB CPM.
HR 773030BD+46 28811925144933213554 D1292620 13 18.0+46 48 574.83 A5IIIn 1.0337.5D:Component D of ADS 13554 of which primary is HR 7735.,N:There is very much confusion in the literature as to which of the three stars HR 7730, 7735, 7751 should be called,N:Omicron1 and which Omricron2:,N:HR FL SOME BAC Others,N:7730 30 Omicron1 Omicron1 -,N:7735 31 Omicron2 Omicron2 Omicron1,N:7751 32 - Omicron3 Omicron2,N:For these stars, the Greek letter is hence omitted from the Name column.,VAR:Delta Sct?
HR 7733BD+42 3642192535493363620I13555 20 13 42.8+43 22 456.14 K4III 6.457.3
HR 7734BD+36 394919253869653 Var?20 14 05.0+36 36 196.45 A0V
HR 773531BD+46 288219257749337757I13554 AV695 Cyg20 13 37.9+46 44 293.79 K2II+B3V 1.0337.5D:Component C, 6.99V, -0.14(B-V), -0.58(U-B) B5V, vsini : 25k/s, at 107" fixed. AP probably single star.,N:See HR 7730.,S:Also classified K4Iab + B4IV-V.,SB:ADS 13554A, 3784.3d, K 14.0k/s, V0 -7.7k/s, msin3i 9.19, asini 711. Unresolved by speckle interferometry. SKYLAB,SB:indicates cool star with hot companion. vsini of secondary 80k/s.,VAR:ADS 13554A, EA 3.77 - 3.88V, 3784.3d. Amp. varies strongly with wavelength. C = NSV 12931, 6.98V.
HR 773629BD+36 395519264069678W V1644 Cyg20 14 32.0+36 48 234.97 A2V 1.6212.4D:B is K1III, optical, vsini =<54k/s.,VAR:Delta Sct 4.94 - 4.97V, 0.031d. Lambda Boo-type star in Delta Sct instability strip.
HR 7737BD+41 36681926594934513572 20 14 21.6+42 06 136.71 B9IV-V 0.20.9D:AB and AC both binary. C, 9v at 12".
HR 774033BD+56 237619269632378758 1293520 13 23.9+56 34 044.30 A3IV-Vn VAR:Delta Sct?
HR 7743BD+33 38271927876970113596 20 15 23.7+33 43 465.66 K0III 6.33.0D:CPM.
HR 775132BD+47 305919290949385IW V1488 Cyg20 15 28.3+47 42 523.98 K3Ib+B3V 5.5208.9N:Originally called Omicron2 Cyg in GCVS, the name has been changed to V1488 Cyg because of much confusion as to,N:which star is Omicron1, which Omicron2. See HR 7730.,S:Also classified K5Iab + B4IV-V and K3II + B9:V.,SB:1147.8d, K 17.0k/s, V0 -5.7k/s, msin3i 9.15, asini 256. Also 390d suspected. Unresolved by speckle,SB:interferometry. SKYLAB indicates cool star with hot companion.,VAR:EA 3.90 - 4.14V, 1147.4d. Period varies. Light var. outside eclipse. The K component may be slightly intrinsically,VAR:variable.
HR 7752BD+38 397719293469720S 20 16 03.4+38 53 526.27 A1V 0.2
HR 7755BD+49 323619298332400S 20 15 43.4+50 13 586.31 R A2Vn 0.2
HR 7756BD+45 311919298549395 20 16 00.6+45 34 465.91 F5V:
HR 7757BD+36 397819298769725 20 16 28.2+37 03 236.48 B6III S:Variously classified from B1III to B8V.
HR 7759BD+39 411419309249410I13640 1298120 16 55.3+40 21 545.24 K3.5IIab-IIb 5.512.8
HR 7762BD+42 367019321749425I 20 17 29.1+42 43 196.29 K4II:
HR 776334BD+37 387119323769773I P Cyg20 17 47.2+38 01 594.81 B2pe G:Cyg OB1.,M:Possible radio source.,RV:Outermost shell RV varies -180 to -240k/s in period 114d. Mass loss 0.0004? solar masses/y.,VAR:SD 3 - 6v. Since 18th century, 4.6 - 5.6v. Shell star, Nova 1600.
HR 7767BD+40 41031933224943813672 20 18 07.0+40 43 565.84 O9V 2.52.6D:AB binary. C, at 34", 11.11V, +0.19(B-V), -0.29(U-B), B7Vp:, vsini 340k/s. D at about 45", 11.17V, +0.19(B-V),,D:-0.32(U-B), B8Vp:, physical, vsini 279k/s. Primary is speckle binary, sep. 0.047".,DYN:0.004".,G:In HII reg. Ma 482.,S:Also classified O8.5V, O8.5III and O9V:((n)).
HR 776936BD+36 399819336969803 20 18 28.6+37 00 005.58 A2V
HR 777035BD+34 3967193370698063627 1299420 18 39.1+34 58 585.17 F5Ib S:IUE observations indicate B8 companion.,SB:2440.0d, K 9.6k/s, V0 -17.3k/s, asini 277.
HR 7777BD+45 313919353649462 V1773 Cyg20 18 49.6+46 19 226.45 B2V SB:2.9847d, K 115.0k/s, V0 -9.1k/s, msin3i 2.84, asini 4.71.,VAR:Amp. 0.05V. Variability agrees with spectroscopic period.
HR 7781BD+54 23291935923245513692 20 18 24.8+55 23 505.76 A2V s 1.33.5D:AB binary. B is dF3.,DYN:0.010".,SB:Both ADS 13692 A and B are SB.
HR 7782BD+36 400819362169841 20 19 48.3+37 07 576.57 A0III S:Shell star. Also classified A1III, A0IV, B9V.
HR 7784BD+38 40211937026985613728 20 20 15.2+39 24 126.23 A1V 1.10.3D:AB 6.33 A2V, 8.87 F6V, 69.86y, a = 0.2766" or 90y, a = 0.214". Component C, 9.2v at 3" also binary with AB.
HR 7786BD+46 291019372249482 V1584 Cyg20 19 56.1+46 50 156.50 B8/9IIIpSi VAR:Alpha CV, amp. 0.04V, 8.5304d. Variable spectrum 1.132854d.
HR 7791BD+53 238419394432491I13743 20 20 30.4+53 35 466.18 K4III 6.26.5
HR 7795BD+40 413619406949524 20 22 03.0+41 07 536.39 G5III+A G:NGC 6910.
HR 7796γ37BD+39 415919409349528765I13765 1304820 22 13.7+40 15 242.20 F8Ib 8.5141.2G:NGC 6910.,M:No physical relation between the radio components and the star. No demonstrable connection between Gamma Cyg and,M:the so-called Gamma Cygni supernova remnant.,N:Sadr; Sador; Sadir.,S:Also classified F0Ia.
HR 7797BD+30 400519409769917I 20 22 37.4+31 15 546.09 K2
HR 7798BD+45 315219415249531 1305020 22 05.4+45 47 425.58 K0III v
HR 7800BD+40 414119419349546I 20 22 45.3+41 01 345.93 K7III
HR 7802BD+42 37211942204955013786 1305320 22 55.5+42 59 006.20 K0III v1.893.2D:AB binary. B, 11v at 1.3". C and D optical.,VAR:ADS 13786B, 8.5 - 11.0V.
HR 780639BD+31 4062194317699503633I 20 23 51.7+32 11 244.43 K2.5IIIFe-0.5 S:Also classified as K3III.
HR 7807BD+37 391619433569951 Var?20 23 44.4+37 28 355.90 B2Ven S:Shell star.
HR 7815BD+53 239719466832534 20 24 32.4+53 33 076.51 B9.5III
HR 7818BD+59 22281948823256213850 20 25 05.1+59 36 006.44 A2IV s 0.30.2D:7.1 A3V, 7.4 A5V, 83.72y, a = 0.172".,S:AB also classified A2IVs.
HR 7823BD+33 391019495170044 20 27 07.7+34 19 446.39 F1II
HR 782640BD+37 394119505070056 20 27 34.3+38 26 255.62 A3V
HR 7827BD+56 24211950663259013870 20 26 23.5+56 38 206.36 B9V 2.026.6D:CPM. Secondary, A2V, vsini 75k/s.
HR 782843BD+48 312819506849643 20 27 02.3+49 23 005.69 dF0 N:Omega Cyg, a case similar to Omicron Cyg (HR 7730): HR, FL, PGC-BAC, Heis-HR; 7828, 43, Omega1, -; 7844,,N:45, Omega2, Omega1; 7851, 46, Omega3, Omega2.
HR 783441BD+29 4057195295700951534I 1311120 29 23.7+30 22 074.01 F5II
HR 783542BD+35 4141195324700961535 20 29 20.4+36 27 175.88 A1Ib
HR 7841BD+45 319619550649704 20 29 59.9+45 55 436.41 K2III
HR 7843BD+55 2411195554326273640W 1311520 29 27.1+56 04 055.91 B9Vne 2.50.8VAR:B component 8.5v, frequently invisible.
HR 7844ω145BD+48 314219555649712364113932 20 30 03.5+48 57 064.95 B2.5IV 7.056.3D:Component B, 12.9v A5V at 18", optical.,G:In reflection nebula.,N:See HR 7828. In the older literature HR 7844 often confused with HR 7851 (q.v.) because the magnitudes and separations,N:of the two brighter components of each, 7844AB, 7851AC, are nearly the same, although the position angles differ. In,N:Allen under the star named Ruchba the P.A. corresponds to HR 7844 while the color clearly refers to HR 7851.
HR 784744BD+36 41051955937013513949 20 30 59.2+36 56 096.19 F5Iab 3.42.0G:Cyg OB1. In reflection nebula; member assoc. Cyg R1 at 1000 pc.
HR 7851ω246BD+48 315419577449741IW 1312820 31 18.8+49 13 135.44 M2IIIab 4.756.8N:See HR 7828, 7844. Ruchba; Rukbat al-dajajah; Al Rukbah al Dajajah.
HR 7854BD+51 288219582032649 20 31 21.1+52 18 356.18 K0III
HR 7860BD+56 244419596432667I 20 31 46.5+56 46 486.14 gK5
HR 7861BD+42 3778195986497723644 20 32 52.3+43 11 306.60 B4III SB:5.3828d, K 31.7k/s, V0 -16.9k/s, asini 2.34.
HR 786647BD+34 407919609370203IW 20 33 54.2+35 15 034.61 K2Ib+B3V 5.6117.6D:AB sep. 0.1", no magnitudes cited. Both 2 micron IR and UV sources.,SB:88.495d, K 20.6k/s, V0 +1.3k/s, asini 17.9. vsini of K2 component =<50k/s, of B3 component <25k/s.
HR 7867BD+41 380519613449796 20 33 48.4+41 46 206.49 K0III-IV
HR 7870BD+46 297719617849804W 20 33 54.9+46 41 385.78 B9pSi 4.1117.7
HR 7876BD+51 2895196379327093646 20 34 50.4+51 51 156.11 A9II
HR 788548BD+31 415919660670287W 20 37 31.8+31 34 216.32 B8IIIn 0.1180.8D:Double with HR 7887 at 181". Third component 12.9v at 71".
HR 7887BD+31 416019662970289W 20 37 32.6+31 31 196.49 F0V 0.1180.8D:Double with HR 7885.
HR 7888BD+37 400219664270288 20 37 23.6+38 19 436.20 K0III
HR 7904BD+29 412119685270323 20 38 59.5+30 20 045.68 K2III
HR 7911BD+40 42661970184989914126 20 39 33.3+40 34 466.06 B6IIIpMn 0.10.8D:AB binary. C, 8.5v A0 at 69" CPM.
HR 7912BD+45 323319703649898 20 39 23.1+45 40 016.58 B5IV
HR 7916BD+55 244419710132763 20 39 00.2+56 00 186.48 R F2Vn VAR:Delta Sct?
HR 7917BD+29 41311971208899714149 20 40 36.2+29 48 196.08 R A2V 4.50.9D:Binary.
HR 7919BD+42 381819713949912 20 40 03.1+43 27 315.95 K2III
HR 792149BD+31 41811971777036214158 20 41 02.6+32 18 265.51 G8IIb 2.32.5D:AB binary.,SB:ADS 14158B, Sp. A. Unresolved by speckle interferometry 1986.45.
HR 7922BD+38 4187197226703673653W 20 41 00.4+39 04 566.51 B6III 3.348.3SB:106.28d, K 14.5k/s, V0 -20.4k/s, e 0.57, asini 17.4.
HR 7924α50BD+44 354119734549941777I14172 Alp Cyg20 41 25.9+45 16 491.25 A2Ia t10.075.4G:Cyg OB7.,N:DENEB; Deneb Cygni; Deneb el Adige; Arided; Aridif; Gallina; Arrioph.,RV:Mass loss 3x10E-10 solar masses/y.,SB:The following two orbits are reported as equally probable: 846.8d, K 3.12k/s, V0 -2.81k/s; 776.4d, K 2.61k/s,,SB:V0 -3.24k/s.,VAR:Alpha Cyg 1.21 - 1.29V. Change in H:H epsilon. No emission recorded before 1944.
HR 7926BD+41 3856197392499463655 20 41 56.5+41 43 015.67 B8II-III
HR 7927BD+34 412719741970406 V568 Cyg20 42 22.2+35 27 226.66 B2IV-Ve G:Runaway star from Lac OB1.,VAR:Gamma Cas 6.40 - 6.68V.
HR 792951BD+49 33531975113280914189 20 42 12.6+50 20 245.39 B2V 6.03.0D:AB fixed.
HR 7932BD+35 423419757270423I X Cyg20 43 24.2+35 35 166.47 F7Ib-G8Ib vVAR:CDelta 5.85 - 6.91, 16.386332d. Period changes.
HR 794252BD+30 416719791270467I14259 20 45 39.7+30 43 114.22 G9.5III 5.06.1DYN:0.020".
HR 7949ε53BD+33 401819798970474780I14274 20 46 12.7+33 58 132.46 K0-III 9.354.9D:AB optical. C, 13v at 78" CPM.,N:Gienah Cygni; Gienah, also applied to HR 4662.
HR 7956BD+33 402819813470499I14290 T Cyg20 47 10.8+34 22 274.92 K3III 6.59.9D:AB CPM. B, 10.03V, +1.27(B-V), +0.66(U-B). C, 13v at 14" optical.,VAR:ADS 14290A, Lb? 4.91 - 4.96V.
HR 7958BD+45 327019815150050W 20 46 38.5+46 31 546.30 A3V 1.90.5
HR 7962BD+52 2799198181328771544 20 46 21.2+52 59 436.33 K0
HR 7963λ54BD+35 42671981837050514296 20 47 24.5+36 29 274.53 B5Ve 1.30.9D:AB 4.85 B5V, 6.07 B7V, 391.30y, a = 0.777". Combined colors. Mag. of blend 4.52V. Component C, 9v K2III-IV at 84",,D:optical; vsini =<54k/s. Resolved by speckle interferometry 1986.45, sep. 0.87".,DYN:0.006".,S:Shell star.,SB:ADS 14296A. Resolved by speckle interferometry 1986.45, sep. 0.05".
HR 7966BD+45 327519823750060I14298 20 47 20.8+45 34 476.40 K3III 6.312.9
HR 7969BD+47 3188198345500733662I14318 20 47 49.3+47 49 555.57 K5III 9.018.3
HR 7972BD+51 29541983873289714322 20 47 52.8+52 24 266.27 G7IV 5.212.2D:Companion optical.
HR 797755BD+45 32911984785009914337 V1661 Cyg20 48 56.3+46 06 514.84 B3Ia e6.321.3D:Optical.,G:NGC 457. Cyg OB7.,RV:4-5d inside atmospheric motion 15-16d. RV results confirmed by H alpha profiles.,VAR:Alpha Cyg 4.81 - 4.87V, no clear periodicity. Small variations in polarization have been observed, 2.0 to 2.6%.
HR 7978BD+51 29571985133290814336 20 48 42.7+51 54 386.29 B8Vnp 2.34.0D:B8V+A3V. CPM.
HR 7983BD+46 30671986255011914350 20 49 54.7+46 39 406.33 B4Ve 5.319.2M:Old disk population runaway star.
HR 798456BD+43 3739198639501213666W 20 50 04.9+44 03 345.04 A4mDel Del 6.075.5G:Hyades moving group.,M:In Schurig's Atlas this is mistakenly labelled 58 Cyg for 56 Cyg.
HR 7996BD+32 397419882070596 20 52 00.3+32 50 576.44 B3III
HR 7999BD+29 422119897689241 20 53 07.4+29 38 586.34 K2
HR 800157BD+43 375519908150180 1338820 53 14.8+44 23 144.78 B5V SB:2.854825d, K 111.9k/s, V0 -21.1k/s, msin3i 2.04, asini 4.34. Apsidal period 203y.
HR 8003BD+44 361719909850182 1339120 53 18.6+45 10 555.45 K0II
HR 8004BD+41 392219909950183 20 53 26.4+42 24 376.66 A1V
HR 8005BD+32 3980199101706453668IW 20 53 53.9+33 26 165.47 gK5 4.0187.7
HR 8009BD+40 43541992185020914413 20 54 22.3+40 42 116.70 B8Vnne 3.95.8D:Fixed sep.
HR 8020BD+46 311119947850246 20 55 49.8+47 25 045.67 B8Ia tG:Cyg OB6; NGC 6991; in reflection nebula IC 5076.,VAR:H alpha profile variable. Possibly binary star.
HR 8022BD+50 323219957833001 20 56 12.9+51 04 306.63 B5V
HR 8023BD+44 363919957950263I 20 56 34.7+44 55 305.96 O6V((f)) C:Color excess E(B-V) = +0.36.,G:Cyg OB7; NGC 7000; exciting star of HII region S117.,S:Also classified O6.5III.,SB:48.608d, K 42.2k/s, V0 -5.8k/s, asini 28.1.
HR 8025BD+50 323319961133004367014460 20 56 25.5+50 43 435.81 F0III 7.77.2D:Binary.,S:Also classified F3Vw.,SB:ADS 14460A.
HR 8026BD+48 324919961250262 20 56 25.9+49 11 455.90 G8II-III
HR 8028ν58BD+40 436419962950274788 20 57 10.4+41 10 023.94 A1Vn
HR 8035BD+43 377719987050298 20 58 19.5+44 28 185.55 K0IIIbFe-0.5 G:Hyades group.,SB:635.1d, K 6.44k/s, V0 -22.63k/s, asini 50.5.
HR 8036BD+41 394919989250303 20 58 30.8+41 56 256.16 B7III SB:15.5143d, K 43.1k/s, V0 -21.7k/s, asini 8.7.
HR 8040BD+49 34261999553303414504 20 58 30.1+50 27 445.61 B5Vn 0.91.8D:AB binary.,DYN:0.003".
HR 804759BD+46 313320012050335155114526 V832 Cyg20 59 49.6+47 31 164.74 B1ne v4.420.1D:AB CPM. B, 9.38V, +0.22(B-V), +0.04(U-B) A8III, vsini 97k/s. Component C, 12v at 26" optical.,G:Cyg OB7.,S:Ultraviolet envelope. Variously classified O9V, B0p, B1IV:e, B1.5Venn, B3ne. Component B, A3V.,VAR:ADS 14526A, Gamma Cas 4.49 - 4.88V. Expanding circumstellar shell. Marked evidence of mass loss. Shell spectrum faded,VAR:between 1973 and 1975. Metallic absorption lines disappeared.
HR 8051BD+35 4357200253707943677 21 01 12.9+36 01 345.97 G5III
HR 805360BD+45 33642003105035914549 V1931 Cyg21 01 10.9+46 09 215.37 B1Ve v4.52.6RV:2.48257d.,S:Shell star. Long-term variation in hydrogen emission.,VAR:5.34 - 5.48V, probably eclipsing; same period as SB.
HR 8062BD+44 367920052750381I 21 02 24.1+44 47 286.19 S4/1III S:Also classified M4SIII = S4/1III.
HR 8063BD+38 432520057770832 21 03 04.8+38 39 276.07 G8III
HR 8064BD+45 33742005955039014585 21 02 48.5+45 50 566.48 B3Vn 0.00.2D:AB, combined mag., colors. CE optical.,DYN:0.002".
HR 8071BD+41 398720072350409W 21 03 52.1+41 37 416.33 F3IV 2.357.3D:AB CPM.,G:In Ursa cluster?
HR 8072BD+49 344820074033091 21 03 26.0+50 21 076.37 K0 G:Hyades group.
HR 8074BD+46 315920075350408 21 03 43.3+46 51 436.32 F0IVn
HR 8078BD+52 2859200817330983682 21 03 47.6+53 17 105.90 K0III
HR 8079ξ62BD+43 380020090550424792I 1351821 04 55.9+43 55 403.72 K4.5Ib-II eD:9.1v A2 companion.,S:Ultraviolet FeII emission.
HR 8084BD+30 4318201078709173687I DT Cyg21 06 30.3+31 11 055.82 F7.5Ib-II vS:Also classified F5.5-F7Ib-II.,VAR:CDelta 5.57 - 5.96V, 2.499215d. Period varies.
HR 808561BD+38 43432010917091979314636 AV1803 Cyg21 06 54.6+38 44 455.21 K5V 0.828.7D:AB 5.22 K5V, 6.04 K7V, 722y, a = 24.65". B is HR 8086. Aa x P, 4.9y, a = 0.014". Astrometric measures indicate 3,D:invisible companions, periods 6, 7 and 12y. Unresolved by speckle interferometry. Suspected planetary companion not,D:substantiated.,DYN:0.300".,G:61 Cyg group.,M:Proper motions for HR 8085 and 8086 taken from Luyten LHS. SAO has only one entry (component A?), but appears to give,M:the mean position of A and B.,VAR:5.19 - 5.27V, 350 - 400d.
HR 808661BD+38 43442010920I14636 B1354621 06 55.3+38 44 366.03 K7V 0.828.7D:See HR 8085.,DYN:0.330".,VAR:ADS 14636B, Is, 6.02 - 6.09V.
HR 808963BD+47 3292201251504563688I14649 1354821 06 36.1+47 38 544.55 K4Ib-IIa 8.315.7
HR 8094BD+29 43242014337096814682 V389 Cyg21 08 38.9+30 12 215.59 B9VpSi 2.33.4D:AB binary. B, 7.8v A0V or Am(A2.5/A7V/A9), vsini 80k/s. C, 9.2v K1III at 58" optical, vsini =<54k/s.,DYN:0.008".,SB:ADS 14682A, 3.3132d, K 20.2k/s, V0 -22.1k/s, asini 0.920. Also about 150d, possibly 110 or 270d.,VAR:ADS 14682A, 5.55 - 5.71V. Alternating periods of 1.12912 and 1.19328d. V 389 Cyg may be triple star, with long period,VAR:about 150d, perhaps 110 or 270d.
HR 8103BD+44 371820173350521 Var?21 09 58.6+45 30 096.63 B4IVpe G:NGC 7039 #170.,S:Shell star.
HR 8105BD+35 44262018197103214724 Var21 11 03.9+36 17 576.54 B1Vp 5.721.5D:Companion B8V.,G:Cyg OB4.
HR 8106BD+52 288020183433185 21 10 15.6+53 33 485.73 B9III
HR 8107BD+47 33222018365053614720 21 10 31.0+47 41 316.46 B6IV e0.8136.1D:AB fixed. B, 9.6v at 1.2". C, 7.29V, +1.55(B-V), +1.38(U-B), M5III, vsini =<25k/s.,S:Spectrum found to display weak double-peaked emission component at H alpha.
HR 8115ζ64BD+29 434820210971070797IW 21 12 56.2+30 13 373.20 G8+III-IIIaBa0.6 7.991.2D:White dwarf companion.
HR 8120BD+36 447020224071086 21 13 26.3+36 38 016.05 F0III
HR 8126BD+29 435420231489549 21 14 10.3+29 54 046.17 G6Ib-IIaCa1Ba0.3
HR 8130τ65BD+37 424020244471121I14787 Tau Cyg21 14 47.5+38 02 443.72 F2IV 2.51.0C:Color excess E(B-V) = +0.09.,D:AB 3.82 F0IV, 6.42 G1V, 49.80y, a = 0.85". Components C, 13v at 29" and P, 12v at 72", both optical. Q, 12v at 90",,D:physical. R, 13v at 90", CPM.,DYN:0.046".,SB:0.143d not confirmed.,VAR:Delta Sct 3.65 - 3.84V. 2-3 hrs.? Possibly variable period.
HR 8136BD+47 334820265450631 21 15 36.8+47 58 256.46 B4IV G:Member of the local association (Pleiades group).
HR 8138BD+41 406720272050656 21 16 29.6+42 15 056.43 R K2
HR 8143σ67BD+38 4431202850711651558 1364021 17 25.0+39 23 414.23 B9Iab vG:Cyg OB4; embedded in dust.,SB:11.043d?,VAR:H alpha profile varies.
HR 8144BD+42 404620286250671 21 17 23.2+42 41 006.19 B7Vn
HR 8146υ66BD+34 437120290471173155914831 Ups Cyg21 17 55.1+34 53 494.43 B2Vne 6.415.3D:AB CPM; 79000?y. Component B, 10.0v G8.5V, probably optical.,G:Cyg OB4.,SB:ADS 14831A. Expanding circumstellar shell.,VAR:4.28 - 4.50V.
HR 8147BD+53 258820292333281 21 17 02.0+53 59 516.13 A1V
HR 815468BD+43 3877203064506903701I V1809 Cyg21 18 27.2+43 56 455.00 O7.5III:n((f)) eG:Cyg OB7; exciting star of HII region S119. Runaway star from Cep OB2 association?,S:Also classified O8V and O8III((f)). H alpha emission moderately intense 1959 to 1970; absorption increasing 1973-1976.,VAR:5.05 - 5.075V, 3.390d.
HR 8155BD+40 44852030965069914849 21 18 55.3+41 02 276.15 A5IV 6.456.
HR 8157BD+37 42712031567120314859 V1334 Cyg21 19 22.2+38 14 155.83 F1II 0.00.1D:Binary, sep. 0.130", about 30y. Unresolved by speckle interferometry.,S:Also classified F2Ib. IUE observations indicate B6-7 companion.,VAR:Delta Cep 5.77 - 5.96V, 3.332816d. Uncertain which component of ADS 14859 is var. Perhaps Delta Sct type.
HR 8161BD+48 3345203245507133702 21 19 28.8+49 30 375.76 B6V
HR 8166BD+31 44252033587123014889 21 20 50.1+32 27 105.68 G8IV 0.42.1D:AB binary. Component B, G5IV.
HR 8169BD+32 413420343971237 21 21 22.0+32 36 466.04 A1V SB:20.30d, K 45.7k/s, V0 -4.0k/s, msin3i 1.88, asini 11.5.
HR 8170BD+39 452920345450739 21 21 01.4+40 20 446.40 F8V G:Sirius group; UMa stream.,SB:3.2434d, K 62.0k/s, V0 +0.4k/s, asini 2.76.
HR 8182BD+29 439720363071259 21 22 41.9+30 18 356.05 K1III
HR 8185BD+48 335720364450761 21 22 00.4+49 23 205.69 K0III
HR 8186BD+38 447120369671266 21 22 46.9+38 38 036.63 A1V
HR 8189BD+36 453720378471276W 21 23 23.0+37 24 246.58 F6II-III 0.0365.4D:Component B of which primary is HR 8193.
HR 8193BD+36 454320385771280W 21 23 48.3+37 21 056.47 R K5 0.0365.4D:Component A in system of which B is HR 8189. Other components 11.6, 13.4, 14.6v.
HR 8206BD+48 33762041315081714962 V1934 Cyg21 24 55.5+49 19 246.58 B9pSi:Cr:Sr: 5.920.3
HR 8208BD+46 330520415350824 21 25 19.6+46 42 525.60 F0V
HR 820969BD+36 45572041727132914969 21 25 47.0+36 40 035.94 B0Ib 5.353.4D:ADS 14969A. Companions optical. B 12.06V, +1.13(B-V), 33". C 10.38V, +0.46(B-V), -0.04(U-B), F5V, 54", vsini =<54k/s.,D:Components B and C sometimes interchanged.,G:Cyg OB4.,S:Nitrogen deficient.
HR 821570BD+36 4568204403713583714 21 27 21.4+37 07 005.31 B3V G:Member of the local association (Pleiades group).,SB:27.54d.
HR 8216BD+48 339020441150867 1371821 26 51.6+48 50 065.31 A6pCrEu: G:Region of NGC 7092.,VAR:Alpha CV?, 5.20 - 5.30V, 0.726d.
HR 8218BD+52 293920442833434 21 26 45.0+52 53 556.03 B6V
HR 8220BD+31 4462204485713713716 21 28 08.3+32 13 315.80 F0V G:Hyades moving group.
HR 822871BD+45 355820477150934807 21 29 27.0+46 32 265.24 K0-III
HR 8237BD+52 295720496533477 21 30 20.4+52 57 296.02 A2Vp S:Lambda Boo star, Mg 4481 wk.
HR 8242BD+51 307920511433497 21 31 27.5+52 37 126.16 G2Ib+B9V S:Cool component also classified G8III. vsini both components =<50k/s.,SB:1322d, K 9.2k/s, V0 -27.0k/s, asini 145.
HR 8246BD+49 355320531451019S 21 32 56.6+49 58 405.75 A0V 0.0
HR 8248BD+45 358420534951027I 1378421 33 17.9+45 51 156.25 K1Ib vC:U-B scatter from +1.850 to +2.05.,G:Cyg OB7.,S:Strong circumstellar components. Unusually high Li content.
HR 8252ρ73BD+44 3865205435510351568I 1378721 33 58.9+45 35 314.02 G8IIIFe-0.5 G:UMa stream.
HR 825572BD+37 4359205512714803722I 21 34 46.6+38 32 034.90 K0.5III
HR 8259BD+51 309120555133540 21 34 27.5+51 41 546.15 B9IIIe
HR 8261BD+29 44562056888983415126 21 36 13.9+30 03 206.36 R G8III-IV 4.42.1
HR 8262BD+44 387720573051079I W Cyg21 36 02.4+45 22 295.53 M5IIIae G:Hyades group.,P:Polarization possibly due to circumstellar dust scattering.,S:Also classified M4e-M6eIII.,VAR:SRb 6.8 - 8.9p, 131.1d; secondary period 235.3d.
HR 826674BD+39 461220583551101811 21 36 57.0+40 24 495.01 A5V
HR 8272BD+44 388920593951109 CP Cyg21 37 27.9+44 41 486.20 A7III VAR:Cst 6.4p.
HR 8275BD+53 265920604033596 21 37 38.7+54 02 326.15 K1III
HR 828475BD+42 4177206330511673730I15208 1383421 40 11.1+43 16 265.11 M1IIIab 4.257.9D:AB binary. B, 10.5v at 3". Component C, optical.,DYN:0.007".
HR 8290BD+54 2595206509336563731 21 40 43.3+54 52 206.20 K0III G:In reflection nebula.
HR 829176BD+40 461120653851189W 21 41 34.3+40 48 196.11 A2V 4.062.1G:Sirius group.
HR 8297BD+34 450020657071613I V460 Cyg21 42 01.1+35 30 376.07 C6.3 VAR:Lb 5.6 - 7.0v. Formerly called DS Peg, now in Cyg.
HR 8298BD+45 363720663251204I V1339 Cyg21 42 08.4+45 45 576.17 M4III: VAR:SRb 5.9 - 7.1v, 35?d.
HR 830077BD+40 461520664451207W 21 42 22.9+41 04 385.69 A0V 0.20.1D:6.4 B9.5V, 6.6 A0V, 27.2y, a = 0.16". ADS 15251 8.3, 8.3, 11.9m at 2' may be member of same system.,DYN:0.017".,SB:Brighter component of visual double. 1.7290d, K 110.0k/s, V0 -25.5k/s, msin3i 0.956, asini 2.62.
HR 8301π180BD+50 3410206672336653733 21 42 05.7+51 11 234.67 B3IV N:Azelfafage.,SB:26.33d, K 16.5k/s, V0 -8.2k/s, asini 5.97.
HR 8304BD+48 348020673151217 21 42 38.9+49 36 016.09 G8II
HR 8306BD+40 462320674951221I 1385721 43 06.4+41 09 185.49 M2IIIab VAR:Lb, 6.3 - 7.08B.
HR 830779BD+37 440820677471643W 21 43 25.7+38 17 025.65 R A0V 1.3151.2D:AB CPM. B is A0. AP, 5.6 11.0v sep. 1.5" binary.
HR 8309μ178BD+28 41692068268994015270 A21 44 08.6+28 44 344.73 H F6V 1.32.0D:AB 4.78 F4V, 6.09 G2V, 507.5y, a = 4.278". B is HR 8310. Combined colors. Mag. for blend 4.50V. Components C, D,,D:optical. D, at 201" is ADS 15275, 6.9 A5, 13.3v sep. 16".,DYN:0.052".
HR 8310μ278BD+28 41692068278993915270 B21 44 08.3+28 44 356.08 H G2V 1.32.0D:See HR 8309.,DYN:0.052".
HR 8320BD+35 4626207088716751571 21 45 44.5+35 51 266.40 G8III
HR 8329BD+42 420420721851277 21 46 16.6+43 03 396.54 G0:III+A4V S:vsini G0 component 100k/s, A4 component =<50k/s.
HR 8335π281BD+48 350420733051293821 21 46 47.6+49 18 344.23 B3III G:Cyg OB7.,SB:72.0162d, K 7.8k/s, V0 -12.3k/s, asini 7.26.
HR 8336BD+35 464320744671716I 21 48 08.3+36 34 506.47 R K5
HR 8338BD+37 442720751671722 21 48 29.4+38 38 556.12 B8V
HR 8345BD+40 4648207673513443745 21 49 40.1+41 08 566.48 A2Ib
HR 8349BD+38 462120785771767 V1619 Cyg21 51 04.9+39 32 126.17 B9pHgMn S:Manganese star. Shows Hg, Mn.,VAR:Alpha CV, amp. 0.01V, 20.70d. Double wave curve. Amplitude var.
HR 8377BD+47 3618208727514773754 21 57 02.2+48 40 076.42 B8V
HR 8403BD+52 3083209419339853763 22 01 50.6+52 52 565.78 B5III G:Member of the local association (Pleiades group).
HR 8407BD+43 41192095155159515578 V1942 Cyg22 02 56.7+44 39 005.60 A0IV 2.51.0D:AB CPM.,G:Sirius group? UMa stream.,S:Also classified B9.5VpCrSiSr.

Revised+Historic NGC/IC, Version 22/9, © Dr. Wolfgang Steinicke [277]
Planetary Nebulae
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 676620 10 23.7+46 27 42PN12.610.90.25planetary, stellarNGC 6884, PK 82+7.1, CS=15.6
NGC 682619 44 48.2+50 31 32PN9.88.80.6planetary, B, pL, R, * 11 MPK 83+12.1, CS=10.4, Blinking planetary
NGC 683319 49 46.6+48 57 42PN13.812.10.18planetary, stellarPK 82+11.1, CS=14.8
NGC 688120 10 52.5+37 24 44PN14.313.90.27planetary, stellarPK 74+2.1, CS=16.7
NGC 689420 16 24.0+30 33 57PN14.412.30.92!!, Ring, F, S, vvlEPK 69-2.1, CS=15.8
NGC 700821 00 32.8+54 32 38PN13.310.71.43cB, L, E 45° ±, r, ** attPK 93+5.2, CS=12.3
NGC 702621 06 18.6+47 51 10PN12.710.90.75pB, biN, planetaryPK 89+0.1, CS=14.5
NGC 702721 07 01.7+42 14 12PN10.48.50.3 × 0.2planetary, stellar = 8.5 mPK 84-3.1, CS=16.3
NGC 704821 14 15.2+46 17 21PN11.312.11.02pF, pL, dif, iR, vlbMPK 88-1.1, CS=18.3
IC 511721 32 31.0+44 35 50PN13.311.50.2Planetary, stellarPK 89-5.1, CS=17.2
Galactic Nebulae
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 685720 01 48.0+33 31 30EN11.40.63F, am Milky Way stPK 70+1.2, Sh2-100, not a PN
NGC 688820 12 06.5+38 21 18EN10.018 × 13F, vL, vmE, ** attLBN 203, Sh2-105, Crescent nebula
NGC 691420 24 43.0+42 29 00RN3 × 3vF, vL, iR, dif, 2 st att pLBN 274
NGC 696020 45 42.0+30 43 00SNR7.070 × 6!! pB, cL, eiF, κ Cygni invLBN 191, Veil nebula
NGC 697420 51 04.0+31 49 54SNRNeb *, neby cE pfknot in Veil nebula
NGC 697920 50 30.0+32 01 36SNR7 × 3vF, S, iE, sev F st f nrpart of Veil nebula
NGC 699220 56 18.0+31 44 30SNR7.060 × 8!!, eF, eL, eE, eiF, bifurcatedCED 182B, Veil nebula
NGC 699520 57 10.0+31 14 00SNR7.012 × 12F, eL, neb & st in groupsCED 182C, Veil nebula
NGC 700020 59 18.0+44 31 00EN4.05.0120 × 100F, eeL, dif nebulosityLBN 373, North America nebula
IC 131820 22 14.0+40 15 24EN50 × 30γ Cygni, surrounded by L patches of F nebyLBN 245, part of Gamma Cyg nebula
IC 1318 A20 16 36.0+41 49 00EN50 × 20γ Cygni, surrounded by L patches of F nebyLBN 251, part of Gamma Cyg nebula
IC 1318 B20 27 54.0+40 00 00EN14.945 × 30γ Cygni, surrounded by L patches of F nebypart of Gamma Cyg nebula
IC 134020 56 08.0+31 02 54SNR25 × 20Possibly conn with h 2093part of Veil nebula
IC 506720 47 50.0+44 22 00EN8.025 × 10FLBN 353, CED 183A, Pelican nebula
IC 506820 50 30.0+42 28 42EN40 × 30vFLBN 328, CED 183B
IC 507020 51 00.0+44 24 06EN8.060 × 50F, difLBN 350, CED 183C, Pelican nebula
IC 507620 55 33.0+47 23 42RN9 × 7vF, vL, lE ns, st invLBN 394, CED 185
IC 514621 53 24.0+47 16 00EN+OCL10 × 10pB, vL, iF, * 9.5 in MOCL 213, LBN 424, Cocoon nebula
Open Clusters
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 681119 37 09.6+46 22 32IV3p6.815Cl, L, pRi, lC, st 11…14OCL 185
NGC 681919 41 18.0+40 11 00I1r7.35Cl, vL, vRi, st 11…15OCL 155
NGC 683419 52 12.5+29 24 29II2m7.86Cl, P, lC, st 11…12OCL 134
NGC 684619 56 28.1+32 20 55IV1p14.20.8eF, vS, 3 st invOCL 139
NGC 686620 03 55.1+44 09 33II2m8.07.67Cl, L, vRi, cCOCL 183
NGC 687120 06 27.0+35 47 24IV3p5.230Cl, st L and S, ** invOCL 148
NGC 687420 07 48.0+38 14 00IV1m7Cl, P, lCOCL 157.1, *Grp ?
NGC 688320 11 18.0+35 51 00I3p8.035Cl, pRi, ** invOCL 152
NGC 691020 23 12.0+40 46 43I2p7.410Cl, pB, pS, P, pC, st 10…12OCL 181
NGC 691320 24 06.0+38 29 36III3p6.610Cl, P, lC, st L and SM 29, OCL 168
NGC 6991 120 55 50.0+47 25 10OCL10Cl, L, P, vlCWH's cluster
NGC 6991 220 54 43.5+47 16 54OCL8Cl, L, P, vlCJH's cluster
NGC 699620 56 30.0+45 28 24III2p10.05Cl, P, lCOCL 197, in Milky Way
NGC 699720 56 30.0+44 39 00III2p10.08Cl, P, lC, st LOCL 197
NGC 703121 06 52.0+50 50 36IV1p9.115Cl of triple st, lCOCL 210
NGC 703921 11 12.0+45 39 00III2p7.615Cl, vL, pRi, E, st 10…OCL 203
NGC 704421 13 09.4+42 29 46II2r12.07Cl, vF, pL, vRi, vC, st 15…18OCL 198
NGC 706221 23 27.4+46 22 43III1p8.35Cl, pS, pRi, pC, st 13…OCL 205
NGC 706321 24 22.0+36 29 12III2p7.09Cl, P, st 10…OCL 192
NGC 706721 24 12.3+48 00 41II2p9.73Cl, P, ? NebOCL 208
NGC 708221 29 17.0+47 07 36IV2p7.224Cl, L, cRi, lC, st 10…13OCL 209
NGC 708621 30 27.5+51 36 02II2m8.412Cl, cL, vRi, pC, st 11…16OCL 214
NGC 709221 31 52.0+48 25 30III2p4.631Cl, vL, vP, vlC, st 7…10M 39, OCL 211
NGC 712721 43 52.9+54 35 46IV1p6Cl, S, P, lCOCL 219
NGC 712821 43 57.7+53 42 55II3m9.74Cl, S, pRi, has a ruby * 9.5OCL 218
IC 131020 10 01.0+34 58 06II1p3F nebyOCL 147, Berkeley 50, in LBN 181?
IC 131120 10 48.0+41 10 24II3rn13.15eF, within circle of stOCL 173, COU 45, URA 50
IC 136921 12 09.0+47 46 00I1m8.85S neb Cl of st 13mOCL 204
IC 499620 16 31.7+37 38 35II3p7.37Cl, st 8...13 (M.N., lxiv.)OCL 158
Galaxies
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 676419 08 16.6+50 55 59SBbc12.611.92.2 × 1.2pF, pL, mE, sev vF st invUGC 11407, MCG 8-35-3, CGCG 256-7, IRAS 19070+5051
NGC 678319 16 47.5+46 01 05C15.414.40.6 × 0.6eF, difficMCG 8-35-7, CGCG 256-13
NGC 679819 24 03.1+53 37 27S014.213.21.6 × 0.9F, vS, R, * v nrIC 1300, UGC 11434, MCG 9-32-2, CGCG 281-1
NGC 680119 27 35.9+54 22 21Sc14.613.91.3 × 0.7eF, pS, R, F * s nrUGC 11443, MCG 9-32-5, CGCG 281-3, IRAS 19264+5416
NGC 682419 43 40.5+56 06 32Sab13.012.21.9 × 1.4pB, iF, bMUGC 11470, MCG 9-32-12, CGCG 281-8, IRAS 19426+5559
NGC 691620 23 33.1+58 20 39SBbc14.313.51.8 × 1.2eeF, pS, F * close p, v difficUGC 11554, MCG 10-29-4, CGCG 304-4, IRAS 20224+5810
NGC 694620 34 52.1+60 09 12SBc9.68.811.5 × 9.8vF, vL, vg, vsbM, rrUGC 11597, MCG 10-29-6, CGCG 304-6, Arp 29, IRAS 20338+5958
NGC 701321 03 33.6+29 53 49S0-a12.411.34 × 1.4pB, cS, R, psbM, pB * npUGC 11670, MCG 5-49-1, CGCG 491-2, IRAS 21014+2941
NGC 711621 42 40.4+28 56 48Sbc14.213.41.1 × 0.4vF, pL, mEUGC 11796, MCG 5-51-1, CGCG 493-5
IC 130119 26 31.9+50 07 33S0-a14.213.31.2 × 0.7eeF, vS, R, 3 st fIC 4867, UGC 11437, MCG 8-35-10, CGCG 256-17, KCPG 539A, NPM1G +50.0429
IC 130219 30 52.8+35 47 06SBc14.113.40.9 × 0.4vF, undefinedMCG 6-43-2, IRAS 19290+3540
IC 130319 31 30.2+35 52 33Sc15.014.31.3 × 0.8vF, S, with S ClUGC 11452, MCG 6-43-4, IRAS 19296+3546
IC 139221 35 32.6+35 23 55E-S013.012.01.1 × 0.7pB, vmbM *UGC 11772, MCG 6-47-3, CGCG 512-6

«Strasbourg-ESO Catalogue of Galactic Planetary Nebulae» Acker et al., 1992 [141]
PNGRADecMain IDPKIRASDiscovererIdentitiesoDiam
["]
rDiam
["]
Dist
[kpc]
Rvel
[km/s]
ExpVel
[km/s]
C* NameC* MagC* SP Type
PN G064.7+05.019 34 45+30 30 59BD+30 363964+05.119327+3024CAMPBELL 1893ARO 11, He 2- 438, VV 235, VV' 503 7.5 8. 0.24 -31.4 ± 0.8 23.0 (O-III), 28. (N-II)AG +30 1906, AG82 376, BD +30 3639, DC 17895, GCRV 11983, HD 184738, LF 2 +30 158, LS II +30 04, PLX 4591B: 11.96, V: 12.50WC 9
PN G066.9+02.219 51 01+31 02 31K 4-3766+02.1KOHOUTEK 1964 12. :
PN G067.9-00.220 03 11+30 32 34K 3-5267-00.120011+3024KOHOUTEK 1964 0. 0.7
PN G068.3-02.720 13 58+29 33 56He 2-45968-02.120119+2924HENIZE 1964ARO 347, VES 123< 5. 1.3 WC 9
PN G068.6+01.119 59 18+31 55 18He 1- 468+01.2HENIZE 1961ARO 191, AS 375, He 2- 453, MHa 92- 31 22.4 +11.6 ± 37.8B: 21.1, V: 21.1
PN G068.7+01.919 56 34+32 22 13K 4-4168+01.119546+3214KOHOUTEK 1964 0. 3.
PN G068.7+03.019 51 53+32 59 18PC 2368+03.119499+3251PEIMBERT et al 1961ARO 165, He 2- 450 5. : 2.1
PN G068.8-00.020 04 44+31 27 26M 1-7568-00.120027+3118MINKOWSKI 1946ARO 168, He 2- 454, VV 248, VV' 524 14.6 -9.0 ± 11.0AG82 396B: >21.
PN G069.2+02.819 54 00+33 22 00K 3-4969+02.119520+3314KOHOUTEK 1964ARO 338< 3. < 0.2
PN G069.2+03.819 50 00+33 45 55K 3-4669+03.119481+3338KOHOUTEK 1964ARO 334 23.
PN G069.4-02.620 16 24+30 33 54NGC 689469-02.120143+3024HERSCHEL 1823ARO 110, HE 2- 460, VV 254, VV' 530 40. 55. 1.5 - 1.9 -58.0 ± 6.0 43.0 (O-III)AG82 404, CSI +30 -20144 2, GCRV 12649, VES 128B: 18.1
PN G069.6-03.920 21 58+29 59 24K 3-5869-03.1KOHOUTEK 1964ARO 348 7.8
PN G069.7-00.020 06 56+32 16 33K 3-5569+00.1KOHOUTEK 1964 5. : 8.2
PN G071.6-02.320 21 04+32 29 24M 3-3571-02.120190+3219MINKOWSKI 1948ARO 172, He 2- 465, VV' 534< 5. 1.5 -176.3 ± 15.1 17.0 (O-III), 30.0 (N-II)AG82 407, GEN +6.20055131, UBV M 44556, VES 131B: >17.6, V: >15.7
PN G072.1+00.120 12 48+34 20 33K 3-5772+00.120108+3411KOHOUTEK 1964< 6. 6.3
PN G073.0-02.420 25 07+33 34 12K 3-76KOHOUTEK 1972 4.3 < 0.2
PN G074.5+02.120 10 52+37 24 43NGC 688174+02.120090+3715PICKERING 1881ARO 108, He 2- 456, VV 250, VV' 526 4. 2.6 > 3.2 -14.4 ± 2.3 16.5 (O-III)AG82 401, CSI +37 -20091, GCRV 12543V: 18.36
PN G075.6+04.320 04 22+39 34 34Anon. 20h02m75+04.1ANON.ARO 342 28.
PN G076.3+01.120 19 56+38 24 31A 6976+01.1ABELL 1955A55 56, ARO 15, VV' 533 22. AG82 406B: >21.
PN G076.4+01.820 17 15+38 50 16KjPn 3KAZARYAN et al 1971K 4-52< 6.
PN G077.5+03.720 12 09+40 50 15KjPn 120107+4038KAZARYAN et al 1971AS 389, K 4-51, MHa 328-107 5.6
PN G077.6+14.719 19 10+46 14 36A 6177+14.1ABELL 1955A55 49, VV' 495 200. -48.0 32. (O-III), > 30. (N-II)AG82 365, CSI +46 -19177, UBV 16374U: 15.82, B: 17.05, V: 17.39
PN G077.7+03.120 15 16+40 40 33KjPn 220136+4025KAZARYAN et al 1971K 3-75 3.5 :
PN G078.3-02.720 42 16+37 40 31K 4-5320403+3729KOHOUTEK 1972 20.
PN G078.6+05.220 08 43+42 30 09Dd 1DOLIDZE 1971K 3-74 20.
PN G078.9+00.720 29 19+40 15 23Sd 1SHERWOOD 1969K 3-77, KjPn 5 7.6 AG82 409
PN G079.6+05.820 09 02+43 43 46M 4-1779+05.120073+4334MINKOWSKI 1948ARO 346 15.2 -26.0 ± 25.0
PN G079.9+06.420 06 55+44 14 21K 3-5679+06.120052+4405KOHOUTEK 1964ARO 345 4.
PN G081.2-14.921 35 29+31 41 45A 7881-14.1ABELL 1955A55 64, ARO 174, VV' 554 107. 0.70 +17.0 ± 10.0 27. (O-III)AG82 433, CSI +31-21334 0, UBV 18570U: 11.86, B: 13.02, V: 13.21O5fek, Of/WR(C)
PN G082.1+07.020 10 24+46 27 39NGC 688482+07.120088+4618COPELAND 1884ARO 57, VV 251, VV' 527 6. 3.1 1.8 -35.6 ± 1.0 23. (O-III)AG82 399B: 16.1, V: >15.6WNb?
PN G082.5+11.319 49 46+48 57 40NGC 683382+11.1PICKERING 1883ARO 105, VV 244, VV' 516 2. 0.5 -108.8 ± 1.7 13. (O-III)AG82 387B: 14.6, V: 14.5
PN G083.5+12.719 44 48+50 31 30NGC 682683+12.119434+5024HERSCHEL 1793ARO 13, VV 242, VV' 514 25. 1.09 -6.2 ± 0.6 11. (O-III)AG +50 1416, AG82 383, BD +50 2869, DC 37693, EM* CDS 1096, GCRV 12124, HD 186924, PLX 4649, SAO 31951, TD1 25412B: 10.33, V: 10.41O3f(H)
PN G083.9-08.421 22 17+38 07 15K 3-81KOHOUTEK 1972 10. : B: 15.49, V: 15.75
PN G084.0+09.520 03 59+49 19 09K 3-73KOHOUTEK 1972 16. B: 20.8
PN G084.2+01.020 45 10+44 39 17K 4-55KOHOUTEK 1972 27.
PN G084.2-04.221 07 40+41 10 57K 3-80KOHOUTEK 1972 5.8
PN G084.9+04.420 32 23+47 21 04A 7185+04.1ABELL 1955A55 58, ARO 352, Sh 2-116, VV' 537 157. 10. (O-III), 20. (N-II)AG82 412, CSI +47 -20308, UBV 17830U: 18.66, B: 19.32, V: 18.95
PN G084.9-03.421 07 02+42 14 10NGC 702784-03.1WEBB 1879ARO 40, Sh 2-113, VV 261, VV' 543 14. 15. 0.94 +8.8 ± 0.6 21.5 (O-III), 23.5 (N-II)AG +42 1976, AG82 421, BD +41 4004, GCRV 13282, HD 201272, PLX 5083, SAO 50463V: 16.25
PN G086.1+05.420 31 53+48 52 41We 1- 10WEINBERGER 1977 190. 26. (O-III), 18. (N-II)AG82 411B: 18.1
PN G086.5-08.821 33 08+39 38 01Hu 1-286-08.121311+3924HUMASON 1921Anon.21h31m, ARO 89, VV 267, VV' 553 8.3 1.7 1.6 -9.0 ± 8.1 29.0 (O-III), 32. (N-II)AG82 432V: 17.32
PN G087.4-03.821 18 07+43 48 40We 2-245WEINBERGER 1977 35.
PN G088.7+04.620 45 23+50 22 40K 3-7820438+5011KOHOUTEK 1972 3.2 4.8
PN G088.7-01.621 14 15+46 17 19NGC 704888-01.121124+4604CURTIS 1919ARO 41, Hb 9, VV 262, VV' 545 61. 70. 1.3 - 2.5 -50.2 ± 8.1 15. (O-III)AG82 424V: 19.12
PN G089.0+00.321 06 18+47 51 07NGC 702689+00.121046+4739COPELAND 1880ARO 59, EM* CDS 1218, VV 260, VV' 542 20. 2.5 -40.6 ± 0.6 38. (O-III), 52.5 (N-II)AG82 420, CSI +47 -21046, HD 201192, PLX 5080B: 15.33, V: 14.20O VI, WC 3
PN G089.3-02.221 19 08+46 18 48M 1-7789-02.121173+4606MINKOWSKI 1946ARO 42, VV 263, VV' 547 7. 8. 2.5 < 6.5 (O-III)B: 12.72, V: 12.12OB ?
PN G089.8-00.621 14 04+47 44 28Sh 1- 8989-00.121123+4733SHARPLESS 1959ARO 357, VV' 544 35. 2.0 7.5 (O-III), 16. (N-II)AG82 423B: 19.7
PN G089.8-05.121 32 31+44 35 48IC 511789-05.121306+4422FLEMING 1905ARO 112, VV 266, VV' 552 1.2 1.5 2.5 -26.1 ± 1.3 16.5 (O-III), 21.5 (N-II)AG82 431, CSI +44-21305 0, EM* CDS 1256, HD 205211B: 17.5, V: 16.7WR
PN G091.6+01.821 10 52+50 47 07We 1- 1121092+5035WEINBERGER 1977 25. AG82 422B: >21.
PN G091.6-04.821 38 49+46 00 30K 3-8421369+4546KOHOUTEK 1972 8.
PN G092.1+05.820 53 14+53 45 43K 3-79KOHOUTEK 1972 11.5
PN G093.3-00.921 30 51+50 00 09K 3-8221291+4946KOHOUTEK 1972 19. 25. 1.9 20. (O-III), 19. (N-II)AG82 428B: 19.5
PN G093.3-02.421 37 01+48 56 12M 1-7993-02.121351+4842MINKOWSKI 1946ARO 365, VV 268, VV'555 33. 30. 2.0 -24.0 ± 25.0 19.0 (O-III), 23. (N-II)AG82 435V: 19.11
PN G093.4+05.421 00 33+54 32 29NGC 700893+05.220590+5420PEASE 1917ARO 39, VV 258, VV' 540 86. 95. 1.3 -74.2 ± 2.0 40.0 (O-III)AG82 417, CSI +54 -20591, GCRV 13203, PLX 5049U: 12.99, B: 13.75, V: 13.23O7, O(H)
PN G093.5+01.421 20 45+51 53 26M 1-7893+01.121190+5140MINKOWSKI 1946ARO 358, VV 264, VV' 548 6.4 3.8 -88.1 ± 1.6
PN G094.5-00.821 35 44+50 54 16K 3-8321339+5040KOHOUTEK 1972 6. : 5.
PN G095.1-02.021 43 18+50 25 15M 2-4995-02.121414+5011MINKOWSKI 1947ARO 367, VV 269, VV' 556< 8. 2.5 -134.0 ± 25.0 12.0 (O-III), 29.5 (N-II)
PN G095.2+00.721 31 50+52 33 52K 3-6295+00.121301+5220KOHOUTEK 1964ARO 362 3. : 2.5 -53.0 ± 4.0 16.0 (O-III)AG82 429Contin.
PN G096.3+02.321 30 01+54 27 30K 3-6196+02.121284+5414KOHOUTEK 1964ARO 361 6.1 6. AG82 427B: >15.9, V: >14.8WC
PN G097.6-02.421 57 42+51 41 41M 2-5097-02.121559+5127MINKOWSKI 1947ARO 368, VV 271, VV' 558 4. 4.5 -136.0 ± 25.0 24.0 (O-III)

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