Constellation Aquila (Eagle)

Aquila
Aquila: IAU Constellation Map [150]

Properties

Aquila is one of the summer constellations. Its brightest star, Atair, marks the well-known summer triangle with Deneb (α Cygni) and Vega (α Lyrae). Sagitta. The star Atair can be easily recognized by its two weaker companions (β and γ Aquilae), who accompany it like bodyguards on the right and left; they are named Alshain and Tarazed, both of which are derived from the Persian name of the constellation, Shahin tara zed (star-studded falcon). This formation is the most striking feature of this constellation, which contains star-rich areas, especially near the southwestern border with Scutum. The area of Aquila is 652 square degrees and it culminates at midnight on around July 12th. [9, 15]

Stars with Proper Names:

  • α Aql: Altair, Atair
  • β Aql: Alshain, Alschairn
  • γ Aql: Tarazed, Reda
  • ε Aql: Deneb El Okab, Deneb
  • ζ Aql: Deneb El Okab, Deneb
Data for constellation Aquila [150]
IAU NameAquila
IAU GenitiveAquilae
IAU Abbr.Aql
English NameEagle
Season (47° N)July … September
Right Ascension18h 41m 18s … 20h 38m 44s
Declination-11° 51' 59" … +18° 41' 18"
Area652 deg2
Neighbours (N↻)Sge, Her, Oph, Ser, Sct, Sgr, Cap, Aqr, Del

Deep-Sky Object Descriptions

Mythology and History

A constellation from ancient times. It had been known as the Adler for over 3000 years. In Greek mythology, the eagle stole Antinous, one of the suitors of Penelope, the wife of Odysseus, and brought him to Olympus, where he became a servant of the gods. The eagle was always at Zeus' side in his long battle against the titans for control of the universe. His job was to carry Zeus' thunder arrows so that he could use them to kill the titans. [73]

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

Aquila also played a role in domestic affairs on Mount Olympus, the seat of the gods. One day the gods needed a new cup carrier to serve them fresh nectar. But this task could only be done by the most beautiful youth on earth. The eagle was sent out to find a new cup-bearer. When he brought the stately Trojan prince Ganymedes to Zeus, the king of the gods was so delighted that he gave the eagle a place under the stars. [73]

An eagle also appears in the Hercules legend. On the way to the tree with the golden apples of eternal youth on the western edge of the earth, Hercules passed a lonely place in the Caucasus. Prometheus, a son of the sky god Uranus and mother earth, lay there forged on a rock. This was the punishment of the gods, since Prometheus created people out of clay for whom he is said to have later stolen the fire from heaven. An eagle came by every day, tore open its body with its pointed, crooked beak and ate at its liver. When Hercules saw this gruesome spectacle, he shot the eagle with an arrow and thus freed Prometheus - at least for a short time - from his torment. An arrow still flies over the constellation Aquila today - did Hercules not hit it after all? [20]

Another version of the first episode is followed by the name The Eagle with the Antinous or Servans Antinoum: The favorite boy of Emperor Hadrian (2nd century AD), an ideal of youthful beauty, was drowned in a river, it is not known whether it was an accident or he drowned himself in order to obtain a long life for his patron Hadrian through this sacrificial death. Shortly afterwards Zeus sent his eagle to lift Antinous up to the starry sky. Many star maps show the boy in the clutches of the eagle and for some time he was listed as a separate constellation south of Aquila. [20, 62]

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 70404BD+01 3766173370123879 1129018 44 49.9+02 03 365.02 B9V eS:Shell star. H alpha emission.,VAR:Gamma Cas?, 5.00 - 5.05V.
HR 70595BD-01 355917365414260611667 18 46 28.5-00 57 425.90 A2Vm 1.612.8D:AB binary, B, Am, F3Vm, or Am(A5/F1/F2), RV +9.2k/s, vsini =<25k/s. C, 11.3v optical.,G:Sirius group; UMa stream.,S:Also classified Am(A1/A7V/A7).,SB:ADS 11667A, spectrum binary, RV var.? Unresolved by speckle interferometry on 1976.30; companion with sep. 0.13" seen,SB:on 1980.48 (McAlister and Hartkopf).
HR 7085BD+00 4027174240123947 18 49 37.1+00 50 096.25 A1V
HR 7099BD+10 3685174569104170I11750 18 50 45.6+10 58 356.55 R K5III+K3III 1.13.5D:Binary, companion K3III-IV.
HR 71018BD-03 43921745891427063500 18 51 22.1-03 19 046.10 F2III
HR 7135BD+06 39781755151240503509I 1153618 55 27.5+06 36 555.57 K0III SB:2994d, K 4.65k/s, V0 +23.31k/s, asini 186.
HR 7143BD-01 36021756401428253510 18 56 22.7-01 48 006.22 B9III S:HgMn star.
HR 7163BD+06 3989176095124112 18 58 23.8+06 14 256.21 F5IV
HR 7165BD+17 379917615510429611884 FF Aql18 58 14.7+17 21 395.38 F8Ib 5.36.6D:Companion blue star?,SB:1435d, K 3.5k/s, V0 -17.4k/s, asini 69.1. RV may also vary in 4109d.,VAR:ADS 11884A, CDelta 5.18 - 5.68V, 4.470916d. Magnetic field. Possible blue companion.
HR 716710BD+13 3838176232104303 V1286 Aql18 58 46.9+13 54 245.89 F0pSrEu G:Sirius group?,S:Oxygen deficient relative to magnesium. Magnetic star. Also classified A4p.,VAR:Alpha CV 5.83 - 5.93V. Published periods of 6.05 and 9.78d probably spurious; nor does a more recent 6.5386d satisfy,VAR:all observations. Period may be years. Abt and Golson found range 5.83 - 5.91V. Two isolated obs. of 5.93 and 5.94V,,VAR:while other observers report intermediate values with amp. <0.015V.
HR 717211BD+13 384117630310430811902 1161818 59 05.7+13 37 215.23 F8V 4.317.8D:Both companions optical.,G:UMa stream.
HR 7173BD+09 3951176304104313 18 59 17.5+10 08 276.75 B2Vp
HR 7176ε13BD+14 3736176411104318712IW 18 59 37.4+15 04 064.02 K1-IIICN0.5Ba0.2 5.9131.1C:V magnitudes scatter from 5.56 to 5.81, B-V from +0.35 to +0.45, U-B from -0.01 to +0.04.,N:Deneb el Okab; Deneb. Names combined with HR 7235.
HR 719312BD-05 4840176678142931I 1165519 01 40.8-05 44 204.02 K1III v
HR 7208BD+08 3951176981124184 19 02 21.6+08 22 276.30 K2III
HR 720914BD-03 4460176984142959W 19 02 54.5-03 41 565.42 A1V 0.00.1D:Sep. 0.099". Consistently unresolved by speckle observations at five epochs between 1977.48 and 1981.47 (McAlister,D:and Hartkopf).,G:Hyades group.
HR 7214BD+01 3865177178124203 19 03 32.2+01 49 085.83 A4V
HR 7219BD+03 3882177332124219 19 04 10.7+03 19 506.73 A5m
HR 7220BD-05 4858177336142985I V Aql19 04 24.2-05 41 066.90 C5II VAR:SRb 6.6 - 8.4v, 10.6 - >12.4p, 353d. Mean mag. varies in cycle of about 2270d.
HR 722515BD-04 4684177463142996I12007 A19 04 57.6-04 01 535.42 K1III 1.638.5D:Companion gK4, optical.
HR 7231BD-01 3642177552143003 19 05 18.6-01 30 466.53 F1V
HR 7235ζ17BD+13 3899177724104461716I12026 1172419 05 24.6+13 51 482.99 A0Vn 8.4158.6DYN:0.020".,G:Pleiades group.,N:Deneb el Okab; Deneb. Combined with HR 7176.
HR 7236λ16BD-05 4876177756143021717I 19 06 14.9-04 52 573.44 B9Vn
HR 7243BD+08 3970177940124266IW R Aql19 06 22.2+08 13 486.09 M7IIIe v5.0180.7S:OH and H2O emission. IR spectra show water vapor. OH, H2O and SiO maser. Also classified M5e-M9e.,VAR:M 5.5 - 12.0v, 284.2d. Period changes 348.980 - 0.554202n + 0.000552309n2 from JD 2399190. Radio flare detected,VAR:in this position.
HR 7245BD+00 4106178065124282 19 07 09.1+00 38 306.56 B9III RV:Period 6.87d.,S:HgMn star.
HR 724818BD+10 37871781251044883525 Y Aql19 06 58.6+11 04 175.09 B8III G:Possible Pleiades group.,SB:1.3023d, K 27.6k/s, V0 -18.7k/s, asini 0.494.,VAR:E 5.02 - 5.06B, 1.30227d. Form of light curve possibly variable.
HR 726619BD+05 40401785961243183530 19 08 59.9+06 04 245.22 F0III-IV
HR 7269BD-00 3662178744143087 19 09 51.6-00 25 416.34 B5Vn
HR 727920BD-08 48871794061431341500 1180819 12 40.7-07 56 225.34 B3V
HR 728721BD+02 3824179761124408353712182 V1288 Aql19 13 42.7+02 17 375.15 B8II-III 7.536.2D:Companion optical.,VAR:Alpha CV 5.06 - 5.16V, 1.73d.
HR 7288BD+05 4081179791124410 1182719 13 44.1+05 30 576.49 A2Vp S:Lambda Boo star, Mg 4481 wk.
HR 7300BD+14 3846180262104655W 19 15 20.1+15 05 015.57 G8II-III 2.189.6D:Binary. Companion A1V.
HR 730322BD+04 4045180482124455 19 16 31.0+04 50 055.59 A3IV
HR 7307BD+14 385218055510466812248 19 16 26.8+14 32 415.63 B9.5V 3.88.2D:AB CPM, B is 9.07V, +0.14(B-V), -0.05(U-B), F8V or G0IV, optical? Speckle interferometry indicates a fourth companion,D:at 0.051" from A.
HR 7313BD+01 3960180782124478 19 17 48.2+02 01 546.19 A1Vn S:High velocity metal-rich subgiant.
HR 7315ω125BD+11 3790180868104691725 19 17 49.0+11 35 435.28 F0IV
HR 731923BD+00 4168180972124487I12289 1188919 18 32.5+01 05 075.10 K2II-III v4.13.1D:AB binary. C, 13.7v at 12" optical.,DYN:0.004".
HR 732124BD+00 4170181053124492W 19 18 50.9+00 20 216.41 K0-IIIa:Ba0.4CH1 0.2423.4
HR 7325BD+09 4057181122124497 19 18 52.7+09 37 056.32 G9III G:Wolf 630 group.
HR 733128BD+12 3879181333104722W V1208 Aql19 19 39.3+12 22 295.53 F0III 3.560.2VAR:Delta Sct 5.51 - 5.57V. Period analyses of new and existing data by Reed and Welch (1988, AJ, 95, 1510) indicate a,VAR:possible change in pulsational modes during the last several years, with fundamental period of 0.146d and possible,VAR:nonradial pulsations of 0.141, 0.183, and 0.091d.
HR 7332ω229BD+11 3802181383104728 19 19 53.0+11 32 066.02 A2V
HR 733326BD-05 49361813911432863544IW 19 20 32.9-05 24 575.01 G8III-IV 6.8115.9D:B probably optical.,M:Possible X-ray source 3U1915-05.,SB:266.544d, K 29.9k/s, V0 -18.0k/s, asini 61.1. High orbital eccentricity, 0.83.
HR 733627BD-01 3716181440143292 19 20 35.7-00 53 325.49 B9III
HR 7347BD-08 4950181858143321 19 22 20.7-08 12 046.31 B3IVp
HR 7349BD-00 37251819071433243546 19 22 21.5-00 15 095.83 gG8
HR 7353BD-07 4942182038143340I 19 23 04.6-07 24 016.32 K0
HR 7354BD+09 40811821011245643548 19 22 48.4+09 54 476.35 F6V
HR 7357BD+14 3896182239104779 19 23 08.2+14 55 166.64 F1V
HR 7366BD-05 4964182475143373 19 25 01.6-04 53 036.52 A9V
HR 737331BD+11 38331825721048071503W 1199419 24 58.2+11 56 405.16 G8IVHdel 1 3.5105.6D:Unresolved by speckle interferometry 1986.46.,G:61 Cyg group.
HR 7377δ30BD+02 3879182640124603730IW 1200419 25 29.9+03 06 533.36 F3IV 7.5108.9D:Component A astrometric binary, A* 3.36 F0IV, 3.422y, a = 0.058"; unresolved by speckle interferometry.,SB:0.1571d.,VAR:Delta Sct? Proper motion slightly variable?
HR 7387ν32BD+00 4206182835124628IW 1202119 26 31.1+00 20 194.66 F2Ib 4.2201.0C:V magnitudes scatter from 4.64 to 4.72, B-V from +0.58 to +0.61, U-B from +0.33 to +0.59.,D:Colors of B are +0.31(B-V), +0.16(U-B).
HR 7389BD+12 3907182900104832 19 26 24.1+13 01 265.74 F6III G:Hyades group.,S:Also classified F7IV and F6V.
HR 7396BD+13 40201831441048623555 1204919 27 33.9+14 16 576.32 B4III
HR 7397BD+02 3892183227124661 19 28 20.8+02 55 495.85 B6III
HR 740035BD+01 4010183324124675 19 29 01.0+01 57 015.80 A0IVp G:In Ursa cluster?,S:Lambda Boo star, Mg 4481, met. wk.
HR 7402BD-07 496818334414345412503 U Aql19 29 21.5-07 02 386.61 F7-G1I-II v5.51.5D:AB fixed. C, 7v at 2", binary.,S:Also classified F5I-II-G1.,VAR:ADS 12503A, CDelta 6.08 - 6.86V, 7.02393d. Period changes.
HR 7404BD-00 3760183387124681I 19 29 18.0+00 14 466.25 K2
HR 7407BD+14 3936183492104896 19 29 22.1+14 35 455.56 K0III
HR 7412BD+02 3904183589124698I12520 1208819 30 10.5+02 54 156.09 K5Ib 4.934.1D:B, optical.
HR 741436BD-03 46121836301434821509I 1209319 30 39.8-02 47 205.03 M1III v
HR 7415BD+03 4043183656124704 V923 Aql19 30 33.1+03 26 406.05 A0eShell S:He lines widened by rotation; NaI lines narrow. Also classified B9.5Ia. Line profiles vary.,VAR:Gamma Cas, amp. 0.12V, 0.8518d. Variation may be due to rotation and inhomogeneous distribution of brightness on disk.
HR 7429μ38BD+07 41321844061247991511I12607 1215519 34 05.4+07 22 444.45 K3-IIIbCN0.5 5.0177.5D:B and C optical.
HR 743037BD-10 51221844921627923562I 19 35 07.3-10 33 375.12 G9IIIa
HR 7432BD-07 4998184573143564 19 35 29.8-07 27 376.34 K0
HR 7438BD+02 3932184663124823 19 35 25.2+02 54 486.38 F6IV
HR 7445BD+10 398118488410503212660 19 36 08.0+11 09 006.68 A3V 6.43.8
HR 7446κ39BD-07 5006184915143600737I 1220419 36 53.5-07 01 394.95 B0.5III G:Sct OB2.
HR 7447ι41BD-01 378218493014359712663 1220119 36 43.3-01 17 114.36 B5III 8.947.0G:Member of the local association (Pleiades group).
HR 7449BD+14 3974184944105036 19 36 15.8+14 23 306.38 K0II-III
HR 7456BD+10 398418501810504512670 19 36 52.5+11 16 245.98 G0Ib 5.780.
HR 746042BD-04 4861185124143621 19 37 47.3-04 38 515.46 F3IV
HR 7471BD+03 40971854231248923569 19 38 49.0+03 22 546.35 B3III
HR 7474σ44BD+05 422518550712490312737 Sig Aql19 39 11.6+05 23 525.17 B3V+B3V v6.647.8D:B, 12v K0Ve at 48" optical. C, 12v at 130". Rotational velocity of A 123k/s, of B 142k/s.,SB:ADS 12737A, 1.950271d, K 164.2k/s, V0 -4.5k/s, msin3i 5.84, asini 4.40. vsini of secondary 129k/s.,VAR:ADS 12737A, EB 5.18 - 5.36B, 1.95026827d. i 71.7d. Spectra vary in period 1.950271d.
HR 748045BD-00 3813185762143678357312775 19 40 43.3-00 37 165.67 A3IV 7.242.0D:A companion at 0.084" discovered by speckle interferometry.
HR 7486BD+13 40981859361051323574W QS Aql19 41 05.5+13 48 566.01 B5V 0.20.1D:Speckle interferometry 1985.5 gives sep. 0.178".,G:Member of the local association (Pleiades group).,SB:2.4968d, K 47.3k/s, V0 -14.2k/s, asini 1.62. Equal components.,VAR:Primary of visual double, EA 5.93 - 6.05V, 2.513294d. Double unresolved in 1961 when period changed sharply.
HR 749346BD+11 3954186122105156 19 42 12.8+12 11 366.34 B9IIIpHgMn
HR 7497χ47BD+11 395518620310516812808 1232519 42 34.0+11 49 365.27 G0:III+A3V 1.20.4D:AB, fixed sep.,DYN:0.0006".,S:Also classified G2+B8 and dF3+A3.
HR 7511ψ48BD+12 4059186547105199 19 44 34.1+13 18 106.26 B9III-IV SB:Double lines suspected.
HR 7516BD-03 47011866601437763579 19 45 52.2-02 53 006.48 B3III
HR 7519υ49BD+07 4210186689125032 19 45 39.9+07 36 485.91 A3IV
HR 7525γ50BD+10 4043186791105223741IW 19 46 15.6+10 36 482.72 K3II e8.0132.6N:TARAZED; Reda.,S:Ultraviolet FeII emission.
HR 7541BD-11 5131187195163012 19 49 02.2-10 52 156.04 K5III
HR 7542BD+10 4058187203105278 19 48 30.4+10 41 396.44 F8Ib-II
HR 7544π52BD+11 399418725910528212962 1242519 48 42.1+11 48 575.72 G2III:+A1V: 0.51.4D:AB, >3000y.
HR 755351BD-11 514918753216303674413017 19 50 46.8-10 45 495.39 F0V 8.021.1D:Optical.
HR 7554BD+07 4252187567125116S V1339 Aql19 50 17.5+07 54 096.51 B2.5IVe 0.1VAR:Gamma Cas? 6.33 - 6.52V.
HR 7557α53BD+08 4236187642125122745I13009 19 50 47.0+08 52 060.77 A7V 8.6165.2D:Component B optical.,N:ALTAIR; Atair.,R:Diam. = 0.00278 - 0.00298".
HR 7559BD-02 5133187660143853I 19 51 11.1-02 27 396.13 K5III
HR 7560ο54BD+10 407318769110533813012 19 51 01.6+10 24 565.11 F8V 8.314.4D:Component B optical. AC, 13.8 dM4, 22" binary.
HR 7562BD+09 4288187753125139 19 51 17.7+09 37 496.25 A1m
HR 7569BD+11 4019187923105348W 1249019 52 03.5+11 37 446.13 G0V 5.590.5
HR 7570η55BD+00 4337187929125159746I Eta Aql19 52 28.4+01 00 203.90 F6Ib vS:Also classified F6Ib-G4Ib. UV suggests A0V companion.,VAR:Discovered by Pigott in 1784. CDelta 3.50 - 4.30V, 7.176641d. Period changes. Variable He 10830 in emission and,VAR:absorption.
HR 7572BD+09 429518796110535513041 1249619 52 15.6+10 21 056.54 B7V 4.013.5D:Component B = A3V.,G:Member of the local association (Pleiades group).
HR 7575BD-03 47421880411438831519 V1291 Aql19 53 18.7-03 06 525.65 A5p vS:Also classified F0p SrCrEu.,VAR:Alpha CV 5.61 - 5.67V, 224.5d. Also period for spectrum and magnetic field var. Rotation 226d.
HR 7580BD+04 4264188107125182 19 53 22.6+04 24 026.53 B9.5Vn
HR 758456BD-08 5150188154143894IW 19 54 08.2-08 34 275.79 gK5 6.146.5
HR 759357BD-08 515418829314389813087 A19 54 37.6-08 13 385.71 B7Vn 0.835.7D:CPM with HR 7594.
HR 759457BD-08 515518829414389913087 B19 54 38.1-08 14 146.49 B8V 0.835.7D:CPM with HR 7593.
HR 7595ξ59BD+08 4261188310125210I 19 54 14.9+08 27 414.71 G9+IIIb
HR 759658BD-00 3871188350125219 19 54 44.8+00 16 255.61 A0III
HR 7598BD+06 435118838512522113093 19 54 40.3+07 08 256.15 A2V 6.413.8D:Optical.
HR 7599BD-07 510218840514391113104 19 55 19.6-06 44 036.51 F2V 1.10.2D:Speckle interferometry 1985.5 gives sep. 0.173".
HR 7602β60BD+06 4357188512125235749I13110 1255719 55 18.8+06 24 243.71 G8IV 7.7175.0D:AB binary. B 12v dM3 at 13".,DYN:0.049".,N:ALSHAIN; Alschairn.,VAR:ADS 13110A, amp. 0.05V.
HR 7610φ61BD+11 40551887281054383590 19 56 14.3+11 25 265.28 A1IV SB:3.3207d, K 37.2k/s, V0 -28.0k/s, asini 1.70.
HR 7636BD+00 43751893221253103596 19 59 22.7+01 22 406.17 G8III
HR 7637BD-10 5238189340163168W 19 59 47.4-09 57 305.88 F8V 0.00.1
HR 7648BD+08 4300189695125355I 20 00 58.9+08 33 295.91 K5III
HR 7661BD-07 5159190172144038 20 04 01.2-07 28 116.72 F4III
HR 7664BD+15 4033190229105615 20 03 30.0+16 01 535.67 B9pHgMn G:Member of the local association (Pleiades group).,N:14 Sge, in Aquila.,RV:61.7d? Earlier vsini 61k/s.
HR 766762BD-01 3887190299144045I 20 04 23.2-00 42 345.68 K4III
HR 7669τ63BD+06 44161903271254031524I 20 04 08.3+07 16 415.52 gK0
HR 7671BD-12 5641190390163245W V1401 Aql20 05 05.4-11 35 586.34 F1III 25. D:Discovered as double by W. Herschel; companion not rediscovered.,S:Probably a supergiant.,VAR:SRd 6.18 - 6.55V, 28.49d.
HR 7680BD+15 4040190658105663I13344 20 05 26.5+15 30 016.34 M2.5III 4.02.7D:CPM.
HR 7681BD-04 5013190664144062 20 06 12.2-04 04 426.47 K0
HR 769064BD-01 3899191067144095 20 08 01.8-00 40 425.99 K1IV
HR 7693BD+08 434419110412547813403 20 07 50.3+09 23 596.43 F3V 2.13.1D:Binary.
HR 7700BD+10 41891912631057433616 20 08 38.3+10 43 336.31 B3V G:Member of the local association (Pleiades group).
HR 7710θ65BD-01 3911191692144150756IW 20 11 18.3-00 49 173.23 B9.5III 9.6113.7G:In reflection nebula.,SB:17.1243d, K 51.0k/s, V0 -27.9k/s, msin3i 0.742, asini 9.52.
HR 7717BD+00 444419198412556713506 A20 12 35.2+00 52 036.27 B9pCrEu:Sr: 0.22.8D:Discordance as to which component has the peculiar spectrum usually attributed to A. However, on the basis of better,D:spectrograms, Abt gives A = A0V, B = A0Vp(Sr,Cr st.,Ca wk.).
HR 772066BD-01 3920192107144181I 20 13 13.9-01 00 345.47 K5III S:Very bright in ultraviolet.
HR 7724ρ67BD+14 42271924251058781526 20 14 16.6+15 11 514.95 A2V
HR 7768BD-01 3951193329144296 20 19 43.3-01 04 436.06 K0
HR 7772BD-06 54511934291443133628I 1301320 20 26.1-06 21 426.63 K5 VAR:Amp. 0.06V.
HR 7794BD+04 44341940131257471531 20 23 10.7+05 20 355.31 G8III-IV
HR 7803BD+00 449519424412576913811 1306420 24 37.5+01 04 076.15 B9V 4.731.3D:Discordances as to which component is B, which C. IDS gives B, 13.1v at 17.1".
HR 7809BD-03 4888194454144412 20 25 42.5-02 48 016.11 gK1
HR 782168BD-03 4906194939144468W 20 28 24.9-03 21 286.13 B9V 7.79.8
HR 783169BD-03 49181951351444951533I 20 29 39.0-02 53 084.91 K2III
HR 787370BD-03 49611963211446243648I 20 36 43.6-02 33 004.89 K5II
HR 7878BD-00 4056196426144632 20 37 18.3+00 05 496.22 B8IIIp
HR 788471BD-01 4016196574144649I14081 1318720 38 20.3-01 06 194.32 G7.5IIIa 7.532.2D:Optical.,SB:ADS 14081A, 205.2d, K 9.8k/s, V0 -5.9k/s, asini 27.7.

Revised+Historic NGC/IC, Version 22/9, © Dr. Wolfgang Steinicke [277]
Planetary Nebulae
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 674119 02 37.0-00 26 56PN10.811.50.13planetary, stellarPK 33-2.1, J 475, CS=14.7
NGC 675119 05 55.5-05 59 30PN12.511.90.43pB, SNGC 6748, PK 29-5.1, CS=13.9
NGC 677219 14 36.4-02 42 22PN14.212.71.43vF, L, R, vvlbM, rPK 33-6.1, CS=18.4
NGC 678119 18 28.3+06 32 25PN11.811.41.9planetary, F, L, R, vsbM disc, S * nfPK 41-2.1, CS=15.0
NGC 678519 18 24.9-01 35 45PN13.312.30.62eS, stellarNGC 6778, PK 34-6.1, CS=15.0
NGC 679019 22 57.0+01 30 49PN10.210.50.17planetary, B, eS, stell = 9.5 magPK 37-6.1, CS=13.5
NGC 680319 31 16.3+10 03 26PN11.311.40.17planetary, stellarPK 46-4.1, CS=15.2
NGC 680419 31 35.4+09 13 33PN12.212.01.1cB, S, iR, rrrPK 45-4.1, CS=14.3
NGC 680719 34 33.5+05 41 04PN13.812.00.13planetary, stellarPK 42-6.1, CS=14.0
NGC 685220 00 39.2+01 43 43PN12.812.60.47F neb, am stPK 42-14.1
IC 484619 16 28.3-09 02 35PN12.711.90.18Planetary, stellarPK 27-9.1, CS=13.7
Open Clusters
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 670918 51 30.0+10 20 00III2m6.715Cl, pRi, lC, iFOCL 100
NGC 675519 07 49.0+04 16 00IV2m7.515Cl, vL, vRi, pC, st 12…14OCL 96
NGC 675619 08 42.5+04 42 21I2m10.64Cl, S, Ri, lC, st 11…12OCL 99
NGC 683719 53 08.0+11 41 54OCL12.03Cl, S, POCL 108
Globular Clusters
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 674919 05 15.3+01 54 05GCL12.44Cl, L, lC, st L & SGCL 107, OCL 91, Berkeley 42, not OCL (I3r)
NGC 676019 11 12.1+01 01 52IX9.09.6pB, pL, vglbM (Auw. 44)GCL 109
Galaxies
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 681419 42 40.5-10 19 28SBbc12.111.23 × 2.8pF, pL, R, bM, rMCG -2-50-1, IRAS 19399-1026
NGC 682119 44 24.2-06 50 04SBcd13.613.11.3 × 1.1F, pL, RMCG -1-50-2, IRAS 19417-0657
NGC 686520 05 56.4-09 02 26S016.015.00.8 × 0.6F, S, E
NGC 690020 21 35.1-02 34 11Sb14.313.51 × 0.8vF, S, RMCG 0-52-1, MCG -1-52-1, IRAS 20189-0243
NGC 690120 22 21.6+06 25 47SBab14.513.71.4 × 0.5eFIC 5000, UGC 11542, MCG 1-52-2, CGCG 399-2, IRAS 20199+0616
NGC 690620 23 34.0+06 26 40SBbc13.212.31.6 × 0.8pF, pL, RUGC 11548, MCG 1-52-3, CGCG 399-6, IRAS 20211+0616
NGC 691520 27 46.0-03 04 36Sab13.012.21.5 × 0.9pB, S, RIRAS 20251-0314
NGC 692220 29 52.8-02 11 30Sc14.013.51.3 × 1vF, pL, RUGC 11574, MCG 0-52-18, CGCG 373-17, IRAS 20272-0221
NGC 692620 33 05.9-02 01 44SBc/P13.212.42 × 1.4vF, pL, E 176°, p of 2UGC 11588, MCG 0-52-33, CGCG 373-33, VV 621, IRAS 20305-0211
NGC 692920 33 21.6-02 02 12S0-a14.413.40.8 × 0.7vF, vS, sf of 2MCG 0-52-35, CGCG 373-35, NPM1G -02.0441
NGC 694120 36 23.5-04 37 08Sb13.612.82 × 1.4eF, lE, lbMMCG -1-52-10, IRAS 20337-0447
IC 131720 23 15.5+00 39 53E114.613.80.7 × 0.6Planetary = * 12, diam 10"-15"UGC 11546, MCG 0-52-4, CGCG 373-5, 2ZW 82
IC 132720 35 41.3-00 00 19S0-a14.914.00.9 × 0.8vF, * 8 1' fCGCG 373-38, KARA 881

«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 G025.9-10.919 18 19-11 06 12Na 226-11.119155-1111NASSAU 1964AS 350, MHa 319- 34, Sa 2-387 16. : AG82 360, AS 350WR
PN G027.6-09.619 16 28-9 02 37IC 484627-09.119137-0908FLEMING 1901ARO 103, AS 348, VV 226, VV' 488, Sa 2-385 2. 2.9 +151.0 ± 3.0 13.1 (O-III)AG82 357, AS 348, BD -09 5069, GCRV 11715, HD 180324B: 15.19, V: 15.19Of
PN G029.2-00.018 44 53-3 20 34TDC 1THOMPSON et al 1991IR 29.211 5.6 6. -55. ± 60.
PN G029.2-05.919 05 56-5 59 28NGC 675129-05.119032-0604FLEMING 1907ARO 101, Sa 2-382, Th 1- J, VV 219, VV' 477 20.5 1.4 -38.5 ± 2.8 40.0 (O-III), 38. (N-II)AG82 344, CSI -06 -19031 0, EM* CDS 1043, HD 177656B: 15.78, V: 15.45WC 4
PN G029.8-07.819 13 56-6 18 51LSA 1LUNDSTROM et a 1988 14.
PN G031.0-10.819 27 02-6 34 54M 3-3431-10.119243-0641MINKOWSKI 1948ARO 322, Sa 2-390, VV' 498 5.6 8. +37.0 ± 25.0 14.0 (O-III)AG82 369B: 16.2, V: 16.3
PN G031.3-00.518 50 25-1 40 09HaTr 10HARTL et al 1983S 2-68 25.
PN G031.9-00.318 50 40-1 03 14WeSb 4WEINBERGER et al 1981 30.
PN G032.0-03.019 00 34-2 11 57K 3-1832-03.118579-0216KOHOUTEK 1964ARO 299, Sa 3-152 4. 0.9
PN G032.5-03.219 02 10-1 48 40K 3-2032-03.218595-0153KOHOUTEK 1964Sa 3-153 0. V: 17.0
PN G032.7-02.018 58 26-1 03 46M 1-6632-02.118558-0107MINKOWSKI 1946Sa 2-378, VV 216, VV' 470< 10. 2.7 +42.6 ± 10.1
PN G032.9-02.819 01 37-1 19 08K 3-1932-02.218590-0123KOHOUTEK 1964ARO 301, Sa 2-379 0. 1.2
PN G033.0-05.319 10 30-2 21 02A 5533-05.119078-0225ABELL 1955A55 43, VV' 480 62. 48. AG82 347B: 20.5
PN G033.1-06.319 14 28-2 42 26NGC 677233-06.119119-0247PICKERING 1879ARO 102, Sa 2-384, VV 224, VV' 486 64. 90. 1.3 :0.0 ± 4.0 10.2 (O-III), 25. (N-II)AG82 355B: 19.02, V: 18.68
PN G033.2-01.918 58 50+0 41 15Sa 3-15118563-0037SANDULEAK 1976 0. B: 14.89, V: 14.00A
PN G033.8-02.619 02 35+0 35 37NGC 674133-02.119000-0031PICKERING 1885ARO 53, J 475, Sa 2-380, VV 217, VV' 474 8. 6. 2.1 +41.3 ± 1.4 23.0 (O-III), 21.5 (N-II)AG82 340B: >20.3
PN G034.0+02.218 45 24+2 01 23K 3-1334+02.118428+0158KOHOUTEK 1964ARO 290 0. 3.7
PN G034.1-10.519 31 07-3 42 24HDW 11HARTL et al 1983HaWe 13 47. AG82 371B: 16.6
PN G034.5-06.719 18 25-1 35 53NGC 677834-06.119158-0141PICKERING 1882ARO 72, Sa 2-388, VV 227, VV' 491 15.8 1.0 +91.0 ± 3.0 20.0 (O-III)AG82 362, CSI -01 -19156, HD 180871, PLX 4502B: 16.91
PN G035.1-00.718 58 08+1 37 06Ap 2-135-00.1APRIAMASVILI 1962ARO 143 32.8 B: 16.96, V: 15.16
PN G035.7-05.019 14 40+0 13 37K 3-2635-05.119120+0008KOHOUTEK 1964ARO 309 10.
PN G035.9-01.119 01 00+2 09 23Sh 2- 7136-01.118594+0204SHARPLESS 1959ARO 31, V-V 1-9, VV'473 100. 114. +24.7 ± 3.0 16.0 (O-III), 21.5 (N-II)AG82 339U: 14.97, B: 14.59, V: 13.75B
PN G036.9-01.119 02 59+3 02 21HaTr 11HARTL et al 1983 12.
PN G036.9-02.619 08 02+2 21 24HaTr 13HARTL et al 1983 21.
PN G037.5-05.119 18 20+1 46 51A 5837-05.119158+0141ABELL 1955A55 45, ARO 150, VV' 489 40. AG82 361, AN 7.1920, C* 2719, NOVA AQL 1919, V605 AqlWC early
PN G037.8-06.319 22 57+1 30 47NGC 679037-06.1PICKERING 1882ARO 33, VV 229, VV' 496 7. 1.8 1.3 +40.4 ± 1.7 15.0 (O-III)AG82 366, BD +01 3979, GCRV 11824, HD 182083, NSV 11959, SON 9934B: 11.1WN?
PN G037.9-03.419 13 07+2 52 49A 5637-03.2ABELL 1955A55 44, ARO 146, VV' 483 181. AG82 352B: 19.7
PN G038.1-25.420 31 33-7 05 21A 7038-25.1ABELL 1955A55 57, ARO 351, VV' 536 42. -79.0 ± 18.0 37.8 (O-III)AG82 410B: 19.1
PN G038.4-03.319 13 23+3 25 03K 4-1938-03.119108+0319KOHOUTEK 1964 0. B: 15.55, V: 14.72
PN G038.7-03.319 13 54+3 37 45M 1-6938-03.219113+0332MINKOWSKI 1946ARO 187, VV 223, VV' 485 0. +7.0 ± 25.0 25.0 (O-III), 30.0 (N-II)
PN G039.5-02.719 13 34+4 38 06M 2-4739-02.119110+0432MINKOWSKI 1947ARO 147, VV 222, VV' 484 6.4 6. +36.0 ± 11.4 11.5 (O-III)AG82 353B: 18.3, V: 17.3
PN G039.8+02.118 56 18+7 07 23K 3-1739+02.118538+0703KOHOUTEK 1964ARO 297 14.8 8.
PN G040.3-00.419 06 46+6 23 56A 5340-00.119043+0619ABELL 1955A55 41, ARO 183, VV' 478 31. AG82 345B: 20.9
PN G040.4-03.119 16 28+5 13 19K 3-3040-03.119140+0507KOHOUTEK 1964ARO 312 0. 3.3
PN G041.2-00.619 09 13+7 05 43HaTr 14HARTL et al 1983 18.
PN G041.8+04.418 51 41+9 54 52K 3-1541+04.118493+0951KOHOUTEK 1964ARO 294 0. < 0.3
PN G041.8-02.919 18 28+6 32 23NGC 678141-02.119160+0626HERSCHEL 1830ARO 32, VV 228, VV' 492 108. 130. 1.6 +4.3 ± 3.7 12.0 (O-III)AG82 363B: 17.10, V: 16.78
PN G042.0+05.418 48 33+10 35 51K 3-1442+05.118461+1032KOHOUTEK 1964AS 324, MHa 352- 9 0. 1. V: 16.2
PN G042.5-14.520 00 40+1 43 52NGC 685242-14.119581+0135KOHOUTEK 1963ARO 167, K 1-18 28. -11.0 ± 5.0 43.1 (O-III)B: 17.70, V: 17.90
PN G042.9-06.919 34 33+5 41 02NGC 680742-06.119320+0534PICKERING 1882ARO 74, VV 234, VV' 502 2. 0.8 -67.7 ± 3.3 13.0 (O-III)AG82 375, BD +05 4196, LF 1 +05 175B: 16.3
PN G043.0-03.019 21 01+7 36 59M 4-1443-03.1MINKOWSKI 1948ARO 120 7.4 7. +48.0 ± 11.0
PN G043.1+03.818 56 33+10 52 14M 1-6543+03.118541+1048MONKOWSKI 1946ARO 142, VV 215, VV' 467 3.6 4.0 +20.0 ± 11.0 11.5 (N-II)AG82 336B: 15.30, V: 14.89
PN G043.3+02.219 02 18+10 17 24PM 1-276PREITE-MARTINEZ 1988CTSS 1 14. B: 19.5, V: 18.5
PN G043.5-13.419 58 29+3 02 23A 6743-13.1ABELL 1955A55 54, ARO 117, VV' 520 67. AG82 390B: 19.3
PN G044.3-05.619 32 39+7 27 58K 3-3644-05.119302+0721KOHOUTEK 1964 12. B: 17.2, V: 17.3
PN G045.4-02.719 24 22+9 53 55Vy 2- 245-02.119219+0947VYSSOTSKY 1945ARO 151, M 1-70, VV 230, VV' 497 14. 0.5 -71.4 ± 3.9 17.5 (O-III), 25.0 (N-II)AG82 367B: 15.51, V: 14.60
PN G045.6+01.519 09 26+12 00 48K 3-2245+01.1KOHOUTEK 1964 0.
PN G045.7-04.519 31 36+9 13 38NGC 680445-04.119291+0907PEASE 1917ARO 34, VV 233, VV' 500 35. 1.1 -12.0 ± 3.8 24.0 (O-III)AG82 373, CSI +09 -19291, HD 183932, PLX 4568B: 14.47, V: 14.37O9, O(H)
PN G045.9-01.919 22 27+10 41 21K 3-3345-01.119200+1035KOHOUTEK 1964 0. 1.1
PN G046.3-03.119 27 45+10 24 21PB 946-03.119253+1018PEIMBERT et al 1960ARO 152 12. : 9.0
PN G046.4-04.119 31 16+10 03 24NGC 680346-04.119289+0956PICKERING 1882ARO 73, VV 232, VV' 499 5.5 2.4 3.0 +13.1 ± 1.8 14.5 (O-III), 20. (N-II)AG82 372, CSI +09 -19289, EM* CDS 1073, HD 183889V: 15.2WN?
PN G046.8+02.919 06 23+13 44 41CTSS 4CAPELLARO et al 1990 10.
PN G046.8+03.819 03 08+14 06 58CTSS 3CAPELLARO et al 1990Sh 2-78 600. B: 17.98, V: 17.78
PN G047.1+04.119 02 40+14 28 52K 3-2147+04.1KOHOUTEK 1964 7.2 B: 18.6, V: 16.9
PN G047.1-04.219 33 18+10 37 01A 6247-04.1ABELL 1955A55 50, ARO 155, VV' 501 161. 13. (O-III), 24. (N-II)AG82 374B: 18.8
PN G048.0-02.319 28 14+12 19 37PB 1048-02.119258+1213PEIMBERT et al 1960Ap 4- 1, ARO 153 10. 8.0
PN G048.1+01.119 15 30+14 03 50K 3-2948+01.219132+1358KOHOUTEK 1964 0. 1.
PN G048.5+04.219 04 51+15 47 36K 4-1648+04.219025+1542KOHOUTEK 1964ARO 303 0. 3.
PN G048.7+01.919 13 38+14 59 30He 2-42948+01.119113+1454HENIZE 1964ARO 148, M 4-13 4.2 +14.0 ± 11.0WC
PN G048.7+02.319 12 06+15 09 01K 3-2448+02.119098+1504KOHOUTEK 1964ARO 305 6.2
PN G048.7-01.519 26 26+13 19 42DeHt 4DENGEL et al 1980 40. AG82 368
PN G049.4+02.419 13 05+15 46 42He 2-42849+02.119108+1541HENIZE 1964ARO 186, M 4-12 9.6 8.
PN G050.4+05.219 04 32+17 57 10A 5250+05.119023+1752ABELL 1955A55 40, ARO 144, VV' 476 37. AG82 342B: 18.4
PN G050.4-01.619 30 17+14 47 22K 4-2850-01.119279+1441KOHOUTEK 1964 0. 0.6
PN G051.0-04.519 42 03+13 50 39PC 2251-04.119397+1343APRIAMASVILI 1959ARO 160, VV' 508 20. : B: 18.8, V: 18.1
PN G051.9-03.819 41 09+14 56 54M 1-7351-03.119388+1449MINKOWSKI 1946ARO 158, He 2- 443, VV 238, VV' 506 5. 6. +6.9 ± 10.1 11.0 (O-III)B: 15.01, V: 14.54
PN G052.2-04.019 42 19+15 09 05M 1-7452-04.119400+1502MINKOWSKI 1946ARO 162, He 2- 445, VV 240, VV' 510< 5. 1.0 +10.0 ± 25.0 12.5 (O-III), 22.0 (N-II)AG82 380B: 18.5, V: 18.1WN b?
PN G052.5-02.919 39 10+15 56 50Me 1-152-02.219368+1549MERRILL 1942ARO 104, He 2- 441, VV' 505, VV 237< 8. 4.7 -6.0 ± 7.0 9.0 (O-III)B: 15.57, V: 14.12
PN G052.9-02.719 39 18+16 21 17K 3-4152-02.119370+1613KOHOUTEK 1964ARO 328 0. 0.5
PN G054.1-12.120 15 09+12 42 07NGC 689154-12.120127+1233COPELAND 1884ARO 37, VV 253, VV' 529 15. 0.83 +42.4 ± 1.0 7.0 (O-III)AG82 403, BD +12 4266, EM* CDS 1140, GCRV 12622, HD 192563B: 12.30, V: 12.42Of (H)

«A Catalog of Parameters for Globular Clusters in the Milky Way» William E. Harris, 1996 [148]
IDNameRADecRSun
[kpc]
RGC
[kpc]
Fe/HwtEB-VVHB(m-M)VVtMV,tU-BB-VV-RV-Isptellipvr
[km/s]
vLSR
[km/s]
sigv
[km/s]
crc
[']
rh
[']
μVρ0lg(tc)lg(th)
GLIMPSE0118 48 49.7-01 29 504.24.904.8528.8028.1522.24-5.911.37 0.590.657.89
NGC 674919 05 15.3+01 54 037.95.0-1.6011.5019.7019.1412.44-6.700.802.14-61.7 ± 2.9-47.20.79 0.621.1021.883.308.598.78
NGC 676019 11 12.01+01 01 49.77.44.8-0.4030.7717.4616.728.88-7.841.091.661.012.12G50.04-27.5 ± 6.3-13.21.65 0.341.2718.663.897.969.01
Pal 1119 45 14.4-08 00 2613.48.2-0.4040.3517.4616.729.80-6.921.27-68.0 ± 10.0-56.00.57 1.191.4619.722.299.619.34

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