Constellation Aquarius (Water Bearer)

Aquarius
Aquarius: IAU Constellation Map [150]

Properties

The constellation Aquarius is in the ecliptic, southwest of the large Pegasusrectangle. The stars in Aquarius are not particularly bright and form a form that is difficult to understand figuratively. The most striking part is probably the y-shaped group of stars with zeta Aquarii in the center, which marks the jug itself. [7] In the southeast corner of the constellation area there are three distinctive star groups, each consisting of 3 to 4 stars, which symbolize flowing water that is snapped up by Piscis Austrinus. The constellation is very large with an area of ​​980 square degrees and extends over three hours in right ascension. The center culminates at midnight on around August 26th. [9, 15]

Stars with Proper Names:

  • α Aqr: Sadalmelik, Sadalmelek, Sadlamulk, El Melik, Saad El Melik
  • β Aqr: Sadalsuud, Sadalsud, Sad Es Saud, Sadalsund, Saad El Sund
  • γ Aqr: Sadalachbia, Sadachbia
  • δ Aqr: Skat, Scheat, Sheat
  • ε Aqr: Albali, Al Bali
  • θ Aqr: Ancha
  • κ Aqr: Situla
Data for constellation Aquarius [150]
IAU NameAquarius
IAU GenitiveAquarii
IAU Abbr.Aqr
English NameWater Bearer
Season (47° N)July … December
Right Ascension20h 38m 19s … 23h 56m 27s
Declination-24° 54' 15" … +03° 19' 32"
Area980 deg2
Neighbours (N↻)Peg, Equ, Del, Aql, Cap, PsA, Scl, Cet, Psc

Deep-Sky Object Descriptions

Mythology and History

The Aquarius constellation is one of the oldest in the sky. Records indicate it was twenty thousand years old. [20] The name goes back to the rainy season among the peoples of the Near East about 2500 years ago. At the height of the rainy season, the sun moved through the constellation and rose with it. [7, 10, 63] The Aquarius was often depicted as a male figure who emptied a water jug ​​to irrigate the land and make it fertile. He was a powerful being and a keeper of the springs. But there is also a relationship to the Assyrian Flood legend, which flowed into the Greek constellations:

Zeus had heard that in the earlier age there was treachery and violence, greed and war, robbery and murder. Then he himself descended to earth, because he could not believe that divine laws are being so disregarded. But he had to convince himself that everything was even worse and more terrible than it had happened to him. «As far as the earth reaches,» he said, «the wild goddess of madness rules and so everyone will receive the punishment they deserve.»

Clouds fell from all over the sky, the grain was whipped to the ground, the gullies of the springs opened and the rivers rolled along without a bank, tearing trees, cattle and people with them. Houses and temples, even towers, disappeared under the rushing floods, there another person climbed a hill, there another boat drove over the ridge of a sunken courtyard. The sea already covered that hill and soon it struck — yes, one could not believe it! — the surf on the peaks of the mountains. Most of the people were swallowed up by the waves, the others died of starvation in the end, lonely.

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

On a two-peaked mountain in Phocis, on Parnassus, a mountain which was sacred to the Muses and Apollo, the little boat, in which Deucalion and his wife Pyrrah had saved themselves, got stuck. They were both innocent and worshipers of the gods. Then Zeus, full of grace, parted the clouds and chased away the rain with the north wind. The tides and currents were called back, the sea regained its shores, the waves disappeared and a devastated earth covered with gray mud remained. Deucalion and Pyrrah were the only ones who spared the great flood. At the altar of Themis they desperately pleaded for advice on how lost humanity, yes, how the sunken world, could be brought back to life. Then a mysterious, dark oracle was bestowed on them: «Go out of the temple, cover your head, loosen the belt of your clothes and throw the bones of the great mother behind you!»

For a long time Deucalion and Pyrrah stood there dismayed because they believed that the oracle required them to violate their love for their parents and to revile, insult and desecrate the shadows of their mothers through a wicked act. Then Deucalion finally understood the meaning of the oracle: The great mother was the earth and the stones were the bones in the body of the earth — and they should throw them behind her!

Without understanding why, they went over, covered their heads, untied their robes and, as ordered, threw the stones behind their backs. The chunks immediately began to lose their hardness and firmness, to soften and shape over time. As soon as they had taken shape and appeared more agreeable, one could see, if indistinctly, the human culture. Since they were not yet pronounced, they were very reminiscent of roughly hewn statues.

What was now partly permeated by some moisture, partly earthy on those stones, was transformed for the benefit of the living body. What was solid and inflexible became bones, but what was a vein in the rock stayed that way and retained its name. After a short time, through the omnipotence of the gods, the stones thrown by the man's hand took on the features of men, and the stones thrown by the hand of women became women again.

So the earth, which had been left desolate and stripped of all life by the flood, was repopulated by people and finally also by animals and plants. In this way Deucalion became the progenitor of a new human race and the constellation of Aquarius is a reminder of this.

In addition to Aquarius (water bearer) there are also the terms amphora (two-handled, narrow-necked clay vessel, tapering at the bottom and thus buried in the earth) and Diota (jug with handle). The transcribed Greek name was Hydrochous and Hydrochoos. [20]

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 7890BD-02 5328196712144666 20 39 13.2-02 24 466.22 B7IIIne vVAR:H alpha varies.
HR 78971BD-00 40641967581260623651I14108 20 39 24.9+00 29 115.16 K1III 7.159.7D:Both companions optical.
HR 7946BD-03 5018197954144802I 20 47 03.6-02 29 126.27 K2
HR 7950ε2BD-10 5506198001144810781 20 47 40.6-09 29 453.77 A1V N:Albali; Al Bali.
HR 79513BD-05 53781980261448141543I EN Aqr20 47 44.2-05 01 404.42 M3III VAR:Lb 4.41 - 4.45V.
HR 7976BD-13 57731984311639243665 20 50 41.8-12 32 425.88 gK1
HR 79824BD-06 560419857114487714360 1335020 51 25.7-05 37 355.99 F5V+F7V 0.91.1D:AB 6.4 F5V, 7.22 F8V, 187y, a = 0.855". Mag., colors for combined light.,DYN:0.019".
HR 79855BD-06 5606198667144889 1336020 52 08.7-05 30 255.55 B9III
HR 7990μ6BD-09 55981987431448951547S 20 52 39.2-08 59 004.73 A3m SB:1782d, K 5.4k/s, V0 -11.4k/s, asini 128.
HR 7994BD-12 5854198802163953S 20 53 05.6-11 34 256.38 G1V 0.2
HR 7998BD-07 5433198949144915 20 53 58.4-06 53 236.44 F1IV
HR 8006BD-01 4075199124144941 EM Aqr20 55 08.1-01 22 246.55 A9Vn VAR:Delta Sct 6.55 - 6.58V, 0.054d. Per. and amp. may vary.
HR 8014BD-04 5307199280144957 20 56 18.3-03 33 416.57 B8Vn
HR 80157BD-10 5553199345144968I14449 1341920 56 54.0-09 41 515.51 gK5 3.5176.6D:AB fixed sep. B, 11.8v at 36".
HR 8017BD-00 413219944212639614457 20 57 10.6+00 27 496.05 K2III 5.426.2D:AB, CPM.
HR 8024BD-15 5848199603164027 DV Aqr20 58 41.9-14 28 586.01 F0IV S:Shell star.,SB:1.5755d, K 95.5k/s, V0 +10.3k/s, asini 2.07.,VAR:EB 5.95 - 6.25V, 1.575531d. Also Delta Sct amp. 0.1V, 0.12d.
HR 804111BD-05 5433199960145022789 21 00 33.8-04 43 496.21 G1V
HR 8054BD-01 4095200340145050 21 02 59.6-00 55 296.50 B6V
HR 8056BD+00 464820037512649114573 21 03 03.0+01 31 556.25 F5V 0.51.3D:AB 6.74 F5, 7.21, 3055y, a = 3.740".,DYN:0.015".
HR 805812BD-06 566420049614506414592 21 04 04.6-05 49 247.31 H A3V 1.92.7D:CPM with HR 8059.
HR 805912BD-06 566420049714506514592 21 04 04.7-05 49 235.89 H G4III 1.92.7D:CPM with HR 8058. Colors for combined light. Mag. for blend 5.54V. Measured sep. Aa 1985.5 0.045" by speckle,D:interferometry.
HR 8068BD+01 44182006631265223681 21 04 45.4+02 16 116.33 G5
HR 8093ν13BD-11 5538201381164182794I 21 09 35.7-11 22 184.51 G8III
HR 8096BD-09 5674201567145171 21 10 46.9-09 21 146.27 K0III
HR 8102BD-15 5908201707164204 EW Aqr21 11 41.3-14 28 206.48 F0Del Del: G:Hyades group.,S:Also classified F0III-IV.,VAR:Delta Sct 6.41 - 6.48V, 0.097d.
HR 8118BD-11 5553202149164240 21 14 16.7-10 36 196.77 B9pHgMn
HR 8121BD-00 4186202259145229I 1361421 14 37.0+00 05 326.38 M1III VAR:Amp. 0.045V.
HR 8132BD-02 5495202554145259 21 16 39.6-01 36 286.48 K0
HR 8134BD-13 5897202606164279 21 17 13.5-13 16 446.40 A2V
HR 814115BD-05 55122027531452783698 21 18 11.1-04 31 105.82 B5V M:Old disk population runaway star.
HR 816016BD-05 5524203222145317 21 21 04.3-04 33 365.87 gG7
HR 817517BD-09 57282035251453513705I 21 22 56.3-09 19 105.99 M0III
HR 818718BD-13 59232037051643641562W 1368421 24 11.5-12 52 415.49 F1V 7.548.9
HR 819220BD-04 5444203843145376 21 24 51.7-03 23 546.36 F0III
HR 819519BD-10 5668203875145382 21 25 13.1-09 44 555.70 F0IV
HR 819921BD-04 54462039261453843708I 21 25 17.0-03 33 245.49 K4III
HR 8203BD-00 4215204041126789 21 25 51.5+00 32 046.46 A1IV
HR 8205BD+00 47262041211267943711 21 26 28.1+01 06 126.13 F5V
HR 8232β22BD-06 5770204867145457808I15050 21 31 33.5-05 34 162.91 G0Ib 7.935.5D:Both companions optical.,G:With Alpha Aqr (HR 8414) and Epsilon Peg (HR 8308) forms an OB triple system. Motion of HR 8232 and 8414,G:(separated by 12d) is nearly perpendicular to the galactic plane.,N:Sadalsuud; Sadalsud; Sad es Saud; Sadalsund; Saad el Sund.
HR 8251BD-04 5489205423145510 21 35 17.6-03 58 595.77 gG9
HR 8263BD-01 418020576514553315142 21 37 33.8-00 23 256.25 A2V 3.331.5D:CPM.,G:UMa stream.
HR 8264ξ23BD-08 57012057671455371569S 21 37 45.1-07 51 154.69 A7V 2.00.1D:Speckle interferometry indicates mag. diff 3.0, sep. 0.033"; D. W. Dunham gives 5.1, 7.1v, 0.07".,SB:8016d, K 11.3k/s, V0 -21.0k/s, asini 1050. Massive invisible component.
HR 827725BD+01 45172060671269653729IW 21 39 33.3+02 14 375.10 K0III 6.3136.8
HR 828726BD+00 4770206445126997I 21 42 10.1+01 17 075.67 K2III G:In Ursa cluster?
HR 8332BD-06 5827207235145671 21 47 38.1-05 55 026.17 A7V
HR 8360BD-04 5568208111145731 21 54 10.4-04 16 345.71 K2III
HR 8363BD-03 532920817714573515432 21 54 35.9-03 18 046.20 F5IV 3.417.6D:Optical.
HR 8376BD-06 5878208703145778 21 58 13.3-05 25 296.33 F5IV
HR 8382BD-05 56742088011457841580 21 58 55.0-04 22 236.22 K2V
HR 839028BD-00 4296209128127235I 22 01 05.0+00 36 185.58 gK4
HR 8394BD-18 60562092401648273761 22 02 11.9-17 54 136.28 gG7
HR 839629BD-17 642220927816483015562 ADX Aqr22 02 26.6-16 57 516.37 A2V+K0III 0.13.6D:Component B, 7.2v, at 3.7" variously classified G2V, G2III:, K0III:; C 11.7v at 143".,SB:0.9450d, K 97.9k/s, V0 +15.0k/s, asini 1.27.,VAR:ADS 15562A, EA 6.37 - 6.78V, 0.9450132d.
HR 840130BD-07 5688209396145836 22 03 16.4-06 31 215.54 K0III
HR 8402ο31BD-02 56812094091458373765 Omi Aqr22 03 18.9-02 09 194.69 B7IVe S:Shell star.,VAR:Gamma Cas 4.68 - 4.89V, 4.57 - 4.65p.
HR 841032BD-01 4242209625145853 22 04 47.4-00 54 245.30 A5m vG:Sirius group? UMa stream.,S:Also classified A8IVm, A9Vm, A8IVms (variable spectrum), A5/A9/F2.,SB:7.8327d, K 6.8k/s, V0 +20.5k/s, asini 0.732.
HR 8414α34BD-01 4246209750145862827IW 22 05 47.0-00 19 112.96 G2Ib v9.0113.0G:See HR 8232.,N:SADALMELIK; Sadalmelek; Sadlamulk; El Melik; Saad el Melik.,VAR:He 10830 possibly variable.
HR 8418ι33BD-14 6209209819164861828 22 06 26.2-13 52 114.27 B9IV-V
HR 843935BD-19 6227210191164888 22 08 59.0-18 31 115.81 B2.5IV
HR 8451BD-04 5623210419145914 22 10 21.1-03 53 396.27 A1Vnn
HR 845238BD-12 61962104241649103771 22 10 37.5-11 33 545.46 B7III
HR 8453BD-04 5625210434145916 22 10 33.8-04 16 026.01 K0III-IV
HR 8457BD-21 6173210464190945 22 11 02.4-21 13 576.09 F6V
HR 846239BD-14 6229210705164923 1406822 12 25.8-14 11 386.03 F2V
HR 8467BD-05 5732210763145940 22 12 43.8-04 43 156.39 F7V
HR 848041BD-21 618021096019098615753 22 14 18.0-21 04 275.32 K0III+F2V 1.65.1D:AB binary. B is F8V.,DYN:0.011".
HR 8495BD-02 5726211356145989 22 16 33.6-01 35 476.15 A5Vn
HR 849642BD-13 6148211361164974I 22 16 48.1-12 49 535.34 gK0
HR 8497CD-2317344211364191021 22 16 59.8-23 08 246.17 G5
HR 8499θ43BD-08 5845211391145991840I 22 16 50.0-07 47 004.16 G8III-IV N:Ancha.
HR 8500BD-09 5948211392145992 1409522 16 52.6-09 02 245.79 gK3
HR 850444BD-06 59602114341459933782 1410022 17 06.5-05 23 145.75 G6III
HR 8507BD-00 4333211575146004S 22 18 04.3-00 14 166.39 F3V 0.1
HR 850845BD-14 6255211676164996 22 19 00.8-13 18 185.95 gG7
HR 8512ρ46BD-08 5855211838146023 22 20 11.9-07 49 165.37 B8IIIpMn:Hg:
HR 851647BD-22 58972120101910831584I 22 21 35.6-21 35 545.13 K2III
HR 8518γ48BD-02 574121206114604484215864 1413222 21 39.4-01 23 143.84 A0V 7.937.4D:Optical.,N:Sadalachbia; Sadachbia.,S:Lambda Boo star.,SB:ADS 15864A. Unresolved by speckle interferometry.
HR 852949CD-2515905212271191105 22 23 30.9-24 45 455.53 gG9
HR 8530BD-07 5765212320146062D 22 23 32.1-07 11 405.93 G6IIIBaII D:Suspected occultation double. Unresolved by speckle interferometry.
HR 853351BD-05 578021240414606715902 22 24 06.9-04 50 135.78 A0V 0.00.3D:AB 6.6 A0, 6.6, 190y, a = 0.490". Measured sep. 0.121" on 1985.5 by speckle interferometry.
HR 853450BD-14 62762124301650443791 22 24 27.1-13 31 465.76 G6.5III
HR 8539π52BD+00 48722125711275201585I Pi Aqr22 25 16.6+01 22 394.66 B1Ve vRV:2-6y.,S:Shell star. Also classified B1III-IVe.,VAR:Gamma Cas 4.42 - 4.70V. Variable magnitude, RV and emission lines due to slow rotation of line of apsides of rapidly,VAR:rotating equatorial shell. Spectrum variable 0.087d. Variable polarization.
HR 8542CD-24171712126431911443793 22 26 10.7-23 40 576.29 A0V
HR 854453BD-17 652021269716507715934 B22 26 34.2-16 44 296.57 H G2V 0.23.3D:Binary with HR 8545. Components C, D, optical.,DYN:0.083".
HR 854553BD-17 652121269816507815934 A22 26 34.4-16 44 336.35 H G1V 0.23.3D:See HR 8544. Colors for combined light. Mag. of blend 5.56V.,DYN:0.083".
HR 8558ζ155BD-00 4365213051146107I15971 B22 28 49.7-00 01 134.59 H F6IV 0.21.8D:Binary with HR 8559, speckle interferometric sep. 1.672" (1982.38). B* 4.51, 12v, 25.5y, a = 0.072".,DYN:0.040".,S:Combined spectrum with HR 8559, F3IV-V.
HR 8559ζ255BD-00 4365213052146108I15971 A22 28 50.1-00 01 124.42 H F3V 0.21.8D:Binary with HR 8558. AB 4.31 F2IV, 4.51 F3IV, 856.0y, a = 5.055". Magnitude for blend 3.65V, combined colors.,D:Component B, HR 8558, is an astrometric binary.,DYN:0.039".
HR 8565BD-13 6204213198165123 22 30 01.5-12 54 546.40 F3IV G:Hyades group.
HR 856756BD-15 6231213236165127 22 30 17.4-14 35 096.37 B8V s S:Hg, Mn. May resemble HR 1339 (53 tau).
HR 8573σ57BD-11 58502133201651341591 22 30 38.8-10 40 414.82 A0IV s G:In Ursa cluster?
HR 8580BD-03 54602134281461363802 22 31 18.4-02 54 406.16 K0
HR 8581BD-07 5797213429146135S 22 31 18.4-06 33 186.14 F7V 0.1
HR 858358BD-11 5855213464165147 22 31 41.3-10 54 206.38 A8III
HR 859060BD-02 5781213789146160W 22 34 02.9-01 34 275.89 G6III 4.498.1
HR 8592υ59BD-21 6251213845191235849 22 34 41.6-20 42 305.20 F4IV
HR 8596CD-2417232213986191246 22 35 36.5-23 59 285.97 gK0
HR 8597η62BD-00 4384213998146181850 22 35 21.4-00 07 034.02 B9IV-Vn
HR 8610κ63BD-04 57162143761462101595IW 22 37 45.4-04 13 415.03 K2III 3.598.3N:Situla.,R:Occultation diameter = 0.0035".
HR 8612BD-08 591221444814621616130 1425522 38 22.2-07 53 526.23 G0III+F0V 1.80.2D:Measured sep. 0.136" on 1985.5 by speckle interferometry.,S:Also variously classified F2 + K0III, G1IV-V, G5III, K0II-III + F.,VAR:ADS 16130. Uncertain which component varies, B-A 0.5 - 1.8v.
HR 8629BD-04 5728214810146239W 22 40 48.0-03 33 156.31 F6V 0.50.3D:AB, 6.4 F8, 7.4 F6, 28.0y, a = 0.17". Speckle interferometric sep. 0.184" on 1985.5153. Occultations indicate third,D:fainter component: sep. 0.129", mag. diff 2.7v 9 Oct. 1973; single 3 Dec. 1973; and 0.065", mag. diff 1.0, 29 Sept.,D:1974. Possibly variable with high orbital motion?
HR 8645BD-09 603821511414627116208 22 43 03.5-08 18 426.45 A5V 1.12.5D:AB binary. B9, A7.
HR 864767BD-07 58382151431462733819 22 43 14.3-06 57 466.41 A0Vn
HR 864966BD-19 6324215167165252I 1429122 43 35.3-18 49 494.69 K4III G:UMa stream.
HR 867068BD-20 64862157211652931597I 22 47 33.1-19 36 485.26 G7III
HR 8673τ169BD-14 634621576616529816268 22 47 42.8-14 03 235.66 A0V 3.923.7D:AB optical.,N:Sometimes called Tau1 Aqr; usually no Greek letter. See HR 8679.
HR 867670BD-11 59232158741653083825 FM Aqr22 48 30.2-10 33 206.19 A9III-IV VAR:Delta Sct 6.16 - 6.19V, 0.087d.
HR 8679τ271BD-14 6354216032165321861IW 1432922 49 35.5-13 35 334.01 M0III 4.5132.5N:Sometimes called Tau2 Aqr; usually without superscript.
HR 8698λ73BD-08 5968216386146362864I Lam Aqr22 52 36.9-07 34 473.74 M2.5IIIaFe-1 eR:Occultation diam. = 0.0074".,S:Ultraviolet FeII emission.,VAR:Lb 3.70 - 3.80V.
HR 870474BD-12 6371216494165359S HI Aqr22 53 28.7-11 37 005.80 B9III 0.50.1D:Mag., colors for combined light. Occultation double 6.7, 6.7v sep. 0.2"; speckle interferometry, sep. 0.076".,S:Hg, Mn.,SB:3.4298d, K 95.3k/s, V0 -7.1k/s, msin3i 1.81, asini 4.49. Shortest known period for an Mn star. Both components,SB:show mercury lines; only primary, manganese.,VAR:Alpha CV, amp. 0.005V. Possible periods 0.724, 1.27, 3.40, 1.70d.
HR 8709δ76BD-16 6173216627165375866 1435622 54 39.0-15 49 153.27 A3V G:Sirius group. Possible Eggen group with HR 63, q.v.,N:Skat; Scheat; Sheat.,S:Also classified A2-4III.
HR 871078BD-07 5886216637146382 22 54 34.1-07 12 176.19 K3III
HR 871177BD-17 6619216640165376 1435822 54 45.5-16 16 195.56 K2.5IIIb
HR 8716BD-05 588521671814638816365 1436022 55 11.0-04 59 165.72 K0III-IV 2.00.6D:120.0y, e 0.68, a 0.47", i 85d, mag. diff 2.0.,VAR:ADS 16365B, 7.6v.
HR 8727BD-05 5894216953146404 22 57 17.2-04 48 366.31 G9III
HR 8741BD-13 6318217251165425I 22 59 35.7-13 04 156.07 K5III
HR 8756CD-23177062174981915853842 23 01 23.0-22 47 276.28 A5V
HR 875781BD-07 5910217531146447I 23 01 23.6-07 03 406.21 K5III
HR 8759BD-05 5910217563146451D 23 01 31.7-04 42 415.94 K0 D:Suspected occultation double.
HR 876382BD-07 5913217701146465I 23 02 32.6-06 34 276.15 M2III G:Wolf 630 group.
HR 8764BD-21 6354217703191604 23 02 44.3-20 52 145.97 K0III-IV
HR 8772BD-05 5917217877146482 23 03 57.3-04 47 436.68 F8V G:Hyades group.
HR 878283BD-08 601821806014649816497 23 05 09.8-07 41 375.43 F2IV+F0V 0.20.2D:AB 6.2 F2Vn, 6.3 F2V, 21.84y, a = 0.200" or 22.0y, a = 0.20". Combined mag., colors. Component C, 84 Aqr, 7.6v K0 at,D:262", optical.,DYN:0.017".,G:Hyades moving group.
HR 8783BD-17 66612180611654813846IW 23 05 12.8-17 04 456.14 K0 5.156.1
HR 878986CD-2417497218240191651I16511 23 06 40.9-23 44 354.47 G9III 10.02.9D:Sep. 2.9" observed 1925; single in 1929.
HR 881288BD-21 6368218594191683873I 23 09 26.8-21 10 213.66 K1III
HR 8816BD-15 63602186391655223856 23 09 49.6-14 30 386.42 A0Vn
HR 881789CD-2317771218640191687IW 23 09 54.8-22 27 274.69 G2IV+A2V 0.80.4S:Also classified G2III + A2V.
HR 8834φ90BD-06 61702192151465851607I 23 14 19.4-06 02 564.22 M1.5III G:Arcturus group.,R:Occultation diam. = 0.0049".
HR 8836BD-11 6032219279165578I16618 23 14 40.2-10 41 196.12 K5III 4.53.5D:AB, CPM.
HR 8840BD-04 58522194021465933860 23 15 34.3-03 29 475.55 A3V
HR 8841ψ191BD-09 61562194491465981608I16633 A23 15 53.5-09 05 164.21 K0III 4.849.2D:BC, 10.0, 10.5v, K3V, 130y, a = 0.6", mean mass BC 0.35 solar. BC combined, 9.19V, +1.03(B-V), +0.93(U-B), CPM with,D:A. Component C is a close double, equal components, showing orbital motion.,G:Variously described as belonging to the 61 Cyg, Epsilon Ind or Zeta Her groups.
HR 8850χ92BD-08 6076219576146612I Chi Aqr23 16 50.9-07 43 365.06 M3III VAR:Lb 4.9 - 5.25V, 6.5 - 6.8p.
HR 8856BD-12 6461219659165609 1448323 17 40.0-11 42 476.34 A1Vn
HR 8858ψ293BD-09 6160219688146620D 23 17 54.2-09 10 574.39 B5V D:Suspected occultation double.
HR 8865ψ395BD-10 6094219832146635160916671 1449123 18 57.7-09 36 394.98 A0V 3.91.4D:AB binary.,G:Hyades group.,VAR:ADS 16671B, 9.0 - >12?v.
HR 886694BD-14 644821983416562516672 A23 19 06.7-13 27 325.08 G5IV 2.40.2D:AB binary. B is K2V. Component A found double by speckle interferometry.,DYN:0.025".,SB:ADS 16672A, 2323.6d, K 5.5k/s, V0 +10.8k/s, asini 175. Unresolved by speckle interferometry 1986.46.
HR 886896BD-05 596621987714663916676 23 19 24.0-05 07 285.55 F3IV-V 4.910.6D:CPM.,G:Hyades moving group.
HR 8869BD-18 62832198791656283868I 23 19 24.1-18 04 315.93 gK3
HR 8879BD-06 6191220035146652D 1451523 20 40.9-05 54 296.17 K0III D:Suspected occultation double.
HR 889097BD-15 640622027816565816708 23 22 39.2-15 02 215.20 A3Vp 0.70.4D:5.6 A2V, 6.4 A7V, 63.16y, a = 0.420".,DYN:0.017".,G:Hyades group.,S:Lambda Boo star, Mg 4481 wk, Ca II st.
HR 889298BD-20 65872203211918581612I 23 22 58.2-20 06 023.97 K0III
HR 8900BD-19 6450220465165672 23 24 07.8-18 41 156.19 G8III
HR 890699BD-21 6420220704191900I 1455423 26 02.8-20 38 314.39 K5III G:Sirius group.
HR 8917BD-12 6496220957165708 23 28 05.2-11 26 596.37 G0V
HR 8921BD-10 6120221081146729I 23 29 00.6-09 15 586.18 K0
HR 8924BD-05 59992211481467363881 1458823 29 32.1-04 31 586.25 K3III v
HR 8928BD-07 6036221308146748 23 31 01.1-06 17 186.39 K0
HR 8931BD-04 5896221356146752 23 31 31.5-04 05 146.49 F8V
HR 8932100BD-22 61412213571919703885 23 31 42.1-21 22 106.29 A9III
HR 8939101BD-21 6437221565191988W 23 33 16.6-20 54 524.71 A1n 2.31.0
HR 8946BD-16 6314221745165780I 23 34 49.4-15 14 455.96 K0
HR 8951BD-08 6142221835146795888 23 35 32.1-07 27 526.39 gG5
HR 8958BD-13 643922209316580416878 23 37 39.6-13 03 375.65 G9IIIFe-0.5 3.931.6
HR 8968ω1102BD-15 6471222345165818 23 39 47.1-14 13 185.00 F0IV
HR 8978CD-2417796222485192083I 1466523 41 07.0-24 09 376.60 M1III VAR:Amp. 0.05(B-V).
HR 8979BD-12 6535222493165828 23 41 08.9-11 40 505.89 G9III G:Probable Hyades group
HR 8980103BD-18 6357222547165834I 23 41 34.5-18 01 385.34 K5III
HR 8982104BD-18 6358222574165836IW 1467123 41 45.8-17 48 594.82 G0Ib-II 2.8120.1
HR 8987BD-16 6345222643165841I 23 42 27.9-15 26 525.28 K4III SB:Unresolved by speckle interferometry 1986.45.
HR 8988ω2105BD-15 647622266116584289416944 23 42 43.3-14 32 424.49 B9.5V 6.05.0D:Component B, CPM, A5Vep; however, the companion is optical.
HR 8992BD-16 6352222800165849I R Aqr23 43 49.5-15 17 046.36 M7IIIpe vS:Strong emission of He 10830 and FeXIII 10747. Spectrum varies M5e-M8.5e + pec.,VAR:M 5.8 - 12.4v, 386.96d. Secular period change, and oscillations in 24y period, also in RV. Variable radio emission,VAR:and SiO maser. May be a symbiotic star embedded in expanding gaseous nebula. Dust cloud associated with red component.,VAR:Companion B2ep may be an accretion white dwarf. Merrill in 1935 and Payne-Gaposhkin in 1946 analyzed the composite,VAR:light curve of R Aqr and its companion, concluding that the companion varies from about 8 to 12p, perhaps by even 5m.
HR 8998106BD-19 65002228471658541621 23 44 12.1-18 16 375.24 B9Vn
HR 9002107BD-19 650622302416586716979 A23 46 00.9-18 40 415.29 F2III+F2V 1.06.6D:11813y, a = 14.21". Companion F2III or F2V, sources discordant; vsini 96k/s.,DYN:0.027".
HR 9009BD-12 6559223170165880 23 47 15.9-11 54 395.73 gK1
HR 9014BD-07 60862233111469193912I 1471523 48 32.5-06 22 506.07 K4III
HR 9021BD-16 6373223428165905 23 49 31.6-15 51 406.24 K2IIIbFe-0.5
HR 9027BD-10 6177223524165911897 23 50 14.7-09 58 275.94 K0IV
HR 9029BD-15 6507223559165915 23 50 33.3-14 24 075.72 K4.5IIIb
HR 9031108BD-19 6522223640165918 ET Aqr23 51 21.3-18 54 325.18 B9pSiSrCr vRV:Binary motion will not account for variations in RV, line profiles or light.,VAR:Alpha CV 5.16 - 5.21V, 3.730d. Variable magnetic field and spectrum.
HR 9037BD-15 6515223774165933 23 52 30.0-14 15 045.87 K3III
HR 9040BD-09 6277223807146953 23 52 50.5-08 59 485.75 K0III
HR 9043CD-2417897223884192218 23 53 20.8-24 13 456.24 A3Shell S:Weak shell absorption; no emission.

Revised+Historic NGC/IC, Version 22/9, © Dr. Wolfgang Steinicke [277]
Planetary Nebulae
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 700921 04 10.8-11 21 47PN8.38.00.58!!!, planetary, vB, S, ellipticPK 37-34.1, CS=11.5, Saturn nebula
NGC 729322 29 38.4-20 50 11PN7.57.317.57! pF, vL, E or biN (Auw 48)PK 36-57.1, ESO 602-PN22, CS=13.5, Helix nebula
Globular Clusters
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 698120 53 27.9-12 32 11IX9.26.6globular, pB, pL, R, gmCM, rrrM 72, GCL 118
NGC 708921 33 27.2-00 49 22II6.616!!, globular, B, vL, gpmbM, rrr, st eSM 2, GCL 121
NGC 749223 08 26.7-15 36 39XII11.24.2eF, L, bet 2 D stGCL 125
Galaxies
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 694520 39 00.5-04 58 20E-S014.413.41.6 × 0.8pF, vS, R, mbMMCG -1-52-15, near SAO 144663
NGC 695920 47 07.2+00 25 49S014.713.70.6 × 0.3vFCGCG 374-13
NGC 696120 47 10.4+00 21 50E214.713.70.6 × 0.5eF, vSCGCG 374-14, NPM1G +00.0554
NGC 696220 47 18.9+00 19 19SBab13.012.12.9 × 2.2cF, S, R, bMUGC 11628, MCG 0-53-3, CGCG 374-15, KCPG 548A, IRAS 20447+0008
NGC 696420 47 24.2+00 18 05E214.013.01.7 × 1.3F, vS, R, bM, * 14 sf ½'UGC 11629, MCG 0-53-5, CGCG 374-17, KCPG 548B
NGC 696520 47 20.5+00 29 03S015.014.00.6 × 0.4vF, vSIC 5058, MCG 0-53-4, CGCG 374-16
NGC 696720 47 34.0+00 24 44S0-a14.013.10.9 × 0.6eF, vS, * 10 50" fUGC 11630, MCG 0-53-6, CGCG 374-18, IRAS 20450+0013
NGC 696820 48 32.4-08 21 35E-S014.313.31.5 × 1.1F, S, R, gbM, F * invMCG -2-53-6, NPM1G -08.0539, IRAS 20458-0829
NGC 697620 52 25.9-05 46 17Sbc14.814.00.8 × 0.7eF, iRNGC 6975, MCG -1-53-15, NPM1G -05.0582, HCG 88C
NGC 697720 52 29.6-05 44 45SBb14.113.21.3 × 0.9vF, S, iRMCG -1-53-16, HCG 88B, NPM1G -05.0583, IRAS 20499-0555
NGC 697820 52 35.4-05 42 40Sb14.113.31.5 × 0.7vFMCG -1-53-17, HCG 88A, IRAS 20499-0554
NGC 698520 45 03.0-11 06 15Sa14.713.81.5 × 0.8eF, vS, iRMCG -2-53-1, VV 546, IRAS 20422-1117
NGC 6985 A20 45 01.4-11 06 29S15.514.70.5 × 0.3eF, vS, iRMCG -2-53-1, VV 546
NGC 700121 01 07.7-00 11 41Sab13.712.91.4 × 1.1eF, S, E 0°UGC 11663, MCG 0-53-16, CGCG 374-37, NPM1G -00.0540, IRAS 20585-0023
NGC 701021 04 39.4-12 20 16E514.013.01.9 × 1eF, pL, R, rIC 5082, MCG -2-53-24, NPM1G -12.0537
NGC 704721 16 27.4-00 49 35SBb14.213.41.2 × 0.7eF, vS, biN pfUGC 11712, MCG 0-54-10, CGCG 375-23, IRAS 21138-0102
NGC 705121 19 51.3-08 46 57Sa13.913.01.4 × 1.1vF, R, gbM, ** nrMCG -2-54-4, IRAS 21171-0859
NGC 706521 26 42.2-06 59 41SBab14.213.41.1 × 0.9vF, sbM, (m has 19m 33s)MCG -1-54-17, NPM1G -07.0504
NGC 7065 A21 26 57.8-07 01 16SBc14.013.11 × 0.9vF, sbM, (m has 19m 33s)MCG -1-54-18, NPM1G -07.0505, IRAS 21242-0714
NGC 706921 28 05.8-01 38 47E-S014.413.41.3 × 0.8vF, S, R, stellUGC 11747, MCG 0-54-19, CGCG 375-40
NGC 707721 29 59.5+02 24 53E114.113.10.8 × 0.7FUGC 11755, MCG 0-54-28, MK 900, CGCG 375-47, ARAK 549, NPM1G +02.0497
NGC 708121 31 24.3+02 29 28Sb13.512.71.3 × 1.3F, S, R, mbM, * 14 sUGC 11759, MCG 0-54-30, CGCG 375-49, KAZ 526, IRAS 21288+0216
NGC 710821 41 53.7-06 42 31E?15.114.11.4 × 0.9vF, S, R, stellNGC 7111, MCG -1-55-2
NGC 712021 44 33.2-06 31 23Sb14.814.00.8 × 0.4vF, S, vlEMCG -1-55-6, IRAS 21419-0645
NGC 712121 44 52.6-03 37 11Sbc14.213.41.1 × 0.6vF, vS, R, vlbMMCG -1-55-8, IRAS 21422-0351
NGC 716421 56 23.5+01 21 52S0-a15.114.20.7 × 0.5eF, R, 4 vF st nCGCG 377-6, NPM1G +01.0536
NGC 716521 59 26.1-16 30 46Sab14.513.70.9 × 0.8eFMCG -3-56-2, IRAS 21567-1645
NGC 716722 00 30.8-24 37 59SBc13.212.51.7 × 1.3F, pS, R, vglbM, * 10 fESO 532-9, MCG -4-52-1, AM 2157-245, IRAS 21576-2452
NGC 717022 01 26.3-05 25 56E-S014.813.81.2 × 0.8vF, pS, iR, bMN, D * p 36 s
NGC 717122 01 01.9-13 16 11SBb12.912.22.6 × 1.5vF, cL, E 124°, vgbMMCG -2-56-5, IRAS 21583-1330
NGC 718022 02 18.5-20 32 52S013.612.61.5 × 0.7vF, S, R, lbM, p of 2ESO 601-6, MCG -4-52-8
NGC 718122 01 43.4-01 57 36S015.014.01 × 0.8eF, vS, stellarCGCG 377-14, NPM1G -02.0476
NGC 718222 01 51.6-02 11 46S0-a15.314.40.9 × 0.4eF, vS, stellarMCG 0-56-6, CGCG 377-15, NPM1G -02.0477
NGC 718322 02 21.2-18 54 56S0-a12.912.03.8 × 1.1vF, pL, E 90°, lbMESO 601-8, MCG -3-56-4, IRAS 21596-1909
NGC 718422 02 39.9-20 48 45SBc11.710.95.9 × 1.3pB, pL, mE 64°, bet 3 st, erESO 601-9, MCG -4-52-9, UGCA 425, IRAS 21599-2103
NGC 718522 02 56.6-20 28 17E/SB013.412.62.3 × 1.5vF, pL, iR, vglbM, f of 2ESO 601-10, MCG -4-52-11
NGC 718822 03 29.0-20 19 03SBbc14.013.21.6 × 0.8eF, pS, E, lbMESO 601-11, MCG -4-52-12
NGC 718922 03 15.9+00 34 17SBb14.313.51 × 0.7F, S, lEUGC 11882, MCG 0-56-7, CGCG 377-17, IRAS 22007+0019
NGC 719822 05 14.1-00 38 52S0/P14.313.31.5 × 1eF, vS, stellarMCG 0-56-8, CGCG 377-23, NPM1G -00.0573
NGC 721122 06 21.8-08 05 22S015.314.31 × 0.7eF, S, stellarNPM1G -08.0602
NGC 721522 08 34.5+00 30 44Sa pec14.913.91.1 × 0.4vF, S, ECGCG 377-31
NGC 721822 10 11.5-16 39 38SBc12.712.02.6 × 1.1pB, lE, rMCG -3-56-8, IRAS 22074-1654
NGC 722022 11 30.9-22 57 11SB014.513.50.9 × 0.7eF, vS, vlE, gbM, * 10 n 3'ESO 532-28, MCG -4-52-20
NGC 722222 10 51.7+02 06 23SBb14.613.81.2 × 1.2vF, SUGC 11934, MCG 0-56-12, CGCG 377-35, NPM1G +01.0542
NGC 723022 14 13.1-17 04 28SBbc14.914.10.9 × 0.9vF, S, R, bMMCG -3-56-12, IRAS 22114-1719
NGC 723922 15 01.3-05 03 10E-S014.813.81.1 × 0.7eF, vSNPM1G -05.0643
NGC 724622 17 42.6-15 34 12Sa15.414.51.5 × 0.8vF, S, vlE, vgbM, * 13 nIC 5198, MCG -3-56-14, IRAS 22150-1549
NGC 724722 17 41.1-23 43 50SBb13.412.61.4 × 0.8pF, vS, R, lbM, B D * p 13sESO 533-8, MCG -4-52-32, IRAS 22149-2358
NGC 725122 20 27.2-15 46 23Sa13.512.61.9 × 1.7F, pS, R, gpmbMMCG -3-57-2, IRAS 22177-1601
NGC 725222 20 44.8-24 40 42SB012.111.42.1 × 1.7F, S, R, erESO 533-15, MCG -4-52-36, Arp 226, IRAS 22179-2455, PRC D-35, AM 2217-245, Atoms for peace galaxy
NGC 725522 23 08.0-15 32 28S0-a15.014.11.3 × 0.4eF, L, mE 30°, sbMNMCG -3-57-6, IRAS 22204-1547
NGC 725622 22 36.0-21 44 05SBb14.013.21.3 × 0.63 F st in F nebNGC 7254, ESO 602-13, KAZ 537, IRAS 22198-2159
NGC 725722 22 36.5-04 07 15SBbc13.512.71.9 × 1.4F, vS, lENGC 7260, MCG -1-57-3
NGC 726622 23 59.0-04 04 23Sa14.313.40.9 × 0.7F, vS, R, alm stellarMCG -1-57-6, MK 910, IRAS 22213-0419
NGC 726922 25 46.8-13 10 01Sb14.513.71 × 0.7eF, pS, R, glbMMCG -2-57-5, IRAS 22231-1325
NGC 728422 28 35.8-24 50 40SB013.112.12.3 × 1.6cF, cS, lE, r, D * invESO 533-31, MCG -4-53-4, VV 74, Arp 93, AM 2224-250
NGC 728522 28 37.8-24 50 26SBa12.811.92.1 × 1.5Neb * 1' dist from h 3943ESO 533-32, MCG -4-53-5, VV 74, Arp 93, AM 2224-250
NGC 7287 A22 28 48.9-22 12 08SB016.015.00.3 × 0.2eF, slightly nebs D *ESO 602-20A
NGC 728822 28 14.9-02 53 05S0-a13.913.02.3 × 1.5vF, eS, stellarMCG -1-57-13, MK 912, IRAS 22256-0308
NGC 729822 30 50.6-14 11 19Sc14.313.71.3 × 1.1vF, pL, iRMCG -2-57-10, MK 1124, IRAS 22281-1426
NGC 730022 30 59.9-14 00 11SBb13.612.92.1 × 1vF, cS, E, vglbMMCG -2-57-11
NGC 730122 30 34.8-17 34 25SBab14.213.41 × 0.5vF, pS, lE, lbMESO 602-23, MCG -3-57-15, VV 372, IRAS 22278-1749
NGC 730222 32 23.9-14 07 15E-S013.212.31.8 × 1.1F, pS, R, vsbMSNIC 5228, MCG -2-57-13
NGC 730822 34 32.0-12 56 01E-S014.713.71.2 × 0.9pB, vS, RIC 1448, MCG -2-57-17
NGC 730922 34 20.6-10 21 22SBc13.012.52 × 1.7vF, pL, R, glbM, rMCG -2-57-16, IRAS 22317-1036
NGC 731022 34 36.8-22 29 06SBbc14.613.80.9 × 0.7vF, pS, R, bMNESO 533-49, MCG -4-53-15, KAZ 544, IRAS 22318-2244
NGC 734122 39 05.6-22 39 59SBab13.112.32.4 × 1pF, pS, E, lbMESO 534-11, MCG -4-53-27
NGC 734422 39 36.1-04 09 32Sab14.513.71.5 × 0.8pF, vS, RMCG -1-57-20
NGC 734922 41 14.7-21 47 48SBb15.114.31 × 0.5eF, vS, E 175°, biN, bnESO 603-4, MCG -4-53-29
NGC 735122 41 26.9-04 26 39S013.912.91.8 × 1pF, pS, R, bM, rMCG -1-57-22
NGC 735922 44 47.9-23 41 17S013.512.52.4 × 0.6pF, vS, pmE, bMNESO 534-22, MCG -4-53-34
NGC 736422 44 24.2-00 09 45S0-a13.512.61.8 × 1.1F, S, R, psbMUGC 12174, MCG 0-58-1, CGCG 379-2
NGC 736522 45 10.0-19 57 06E-S013.712.91.5 × 1vF, eS, R, gbMN, * 11 nf 4'ESO 603-10, MCG -3-58-1, NPM1G -20.0607
NGC 737122 46 03.6-11 00 02SB0-a12.311.52 × 2vF, pL, R, lbMMCG -2-58-1, NPM1G -11.0516
NGC 737722 47 47.4-22 18 41SB0-a12.111.13 × 2.5pB, S, vlE, vgmbM, * 12 pESO 534-26, MCG -4-53-38, IRAS 22451-2234
NGC 737822 47 47.5-11 49 00SBab13.512.71.5 × 0.9vF, pLMCG -2-58-5
NGC 738122 50 08.1-19 43 29Scd14.914.20.7 × 0.5eF, vS, R, gbMESO 603-17, MCG -3-58-7A
NGC 739122 50 36.0-01 32 41E113.111.91.7 × 1.5cF, cS, R, sbM * 13, * npUGC 12211, MCG 0-58-6, CGCG 379-8
NGC 739222 51 48.6-20 36 31SBbc12.611.92.2 × 1.4pB, pS, lE 120°, mbMESO 603-22, MCG -4-53-40
NGC 739322 51 38.2-05 33 26SBc/P13.612.92 × 0.9vF, pL, lE, vgbM, rMCG -1-58-2, VV 68, Arp 15
NGC 739922 52 39.3-09 16 03S0-a14.613.70.9 × 0.4eF, pLMCG -2-58-6
NGC 740622 53 56.4-06 34 44S?14.513.61.1 × 0.6F, S, lEMCG -1-58-3
NGC 741622 55 41.6-05 29 42SBb13.212.43.2 × 0.7F, pL, pmE, vgbMMCG -1-58-4
NGC 742522 57 15.6-10 57 00SB0-a15.114.20.9 × 0.6eF, vlE, * 10 p 4'MCG -2-58-13
NGC 744122 56 41.4-07 22 47Sc14.513.81.3 × 0.8vF, pS, iR, * 10 p (? PD)IC 1458, MCG -1-58-7
NGC 744323 00 08.7-12 48 28S0-a12.611.61.4 × 0.5F, vS, vlE, smbM, er, n of 2MCG -2-58-15
NGC 744423 00 08.8-12 50 03S013.912.91.7 × 0.6F, vS, vlE, smbM, er, s of 2MCG -2-58-16
NGC 745023 00 47.7-12 55 04S0-a14.013.11.8 × 1.8vF, SMCG -2-58-19, MK 1126
NGC 749123 08 06.0-05 57 59Sbc14.613.81 × 0.7vF, S, R, vlbMMCG -1-59-2, IRAS 23054-0614
NGC 749423 08 58.4-24 22 09E115.614.60.8 × 0.7eF, vS, stellarESO 535-5, MCG -4-54-7
NGC 749823 09 56.0-24 25 28Sab15.214.40.9 × 0.4vF, S, iRESO 535-6, MCG -4-54-8
NGC 752023 12 53.1-23 28 08Sa14.113.21.3 × 0.8F, pS, bet 2 stIC 5290, ESO 535-8, MCG -4-54-14
NGC 757323 16 26.3-22 09 14SBc14.513.71.3 × 1.1eF, S, iR, b np, * 10 p 4'ESO 604-8, MCG -4-54-17, NPM1G -22.0395, AM 2313-222
NGC 757623 17 22.7-04 43 40S0-a13.712.91.3 × 0.9F, S, smbMMCG -1-59-12, IRAS 23148-0500
NGC 758523 18 01.3-04 39 01S0-a12.311.42.3 × 2pB, pS, iR, gbMMCG -1-59-15, Arp 223
NGC 759223 18 22.0-04 24 59S0-a14.413.51.1 × 0.9eF, vSMCG -1-59-17, MK 928, VV 731, IRAS 23157-0441
NGC 759623 17 12.0-06 54 42S015.214.21 × 0.5vF, pS, lE 0°, lbMNIC 1477, MCG -1-59-11, IRAS 23145-0711
NGC 760023 18 53.8-07 34 48E-S012.912.02.5 × 1cF, S, R, psmbMMCG -1-59-19
NGC 760623 19 04.8-08 29 11Sb11.510.85.4 × 2.1pF, cL, pmE 0° ±MCG -2-59-12, IRAS 23164-0845
NGC 764623 24 06.9-11 51 37Sc14.013.30.9 × 0.6vF, vS, E 260° (neb?), * 9 n 3'.6IC 5318, MCG -2-59-15, IRAS 23215-1208
NGC 765623 24 31.5-19 03 33S014.513.51.2 × 1.1vF, vS, R, bMNESO 605-5, MCG -3-59-8, VV 669, NPM1G -19.0676
NGC 766523 27 14.8-09 23 11Sm13.913.30.7 × 0.7eF, S, stellarMCG -2-59-19, IRAS 23246-0939
NGC 769223 32 46.7-05 35 46Irr15.414.80.5 × 0.4Neb, * 9 f 18s, 73" sMCG -1-60-3, IRAS 23302-0552
NGC 770923 35 27.2-16 42 20SB013.612.62.3 × 0.6pF, S, R, lbMMCG -3-60-2, IRAS 23328-1658
NGC 771723 37 43.6-15 07 07SB0-a13.712.81.4 × 1.2vF, SMCG -3-60-8
NGC 7719 123 38 02.6-22 58 29Sab15.014.20.9 × 0.7eF, vS, RESO 536-12, IRAS 23354-2315
NGC 7719 223 38 02.5-22 58 40S17.016.20.2 × 0.1eF, vS, R
NGC 772123 38 48.6-06 31 04Sc12.211.62.8 × 1.1pF, cL, E 12° ±, vgbMMCG -1-60-17, IRAS 23362-0647
NGC 772323 38 57.0-12 57 40SBb11.911.23.5 × 2.2cB, cL, E, gmbM, rMCG -2-60-5, IRAS 23363-1314
NGC 772423 39 07.0-12 13 27Sb13.712.91.5 × 1eF, pL, iRMCG -2-60-6
NGC 772523 39 14.7-04 32 20S014.813.80.8 × 0.7eeFMCG -1-60-18, IRAS 23367-0448
NGC 772723 39 53.7-12 17 34SBa/P11.510.64.7 × 3.5pB, pL, iR, mbMMCG -2-60-8, VV 67, Arp 222, IRAS 23367+2651
NGC 773023 40 45.8-20 30 32Sc14.914.00.7 × 0.6pB, pL, EESO 606-2, MCG -4-55-22, IRAS 23381-2047
NGC 773623 42 25.7-19 27 09S013.912.91.7 × 1.5eF, eS, gbM, bet 2 st 12ESO 606-5, MCG -3-60-10, NPM1G -19.0695
NGC 775423 49 11.2-16 36 02Sa15.414.50.6 × 0.3eF, vSMCG -3-60-21, IRAS 23466-1652
NGC 7754 A23 49 06.4-16 34 45S016.515.50.4 × 0.2eF, vS
NGC 775823 48 55.1-22 01 27E/SB015.114.10.7 × 0.5eF, vS, iR, sbM, D * 10 nf 50sESO 606-10, NPM1G -22.0413
NGC 775923 48 54.6-16 32 27SB014.013.01.3 × 0.9vF, S, R, lbM, B * nMCG -3-60-18
NGC 7759 A23 48 56.8-16 32 26S15.614.80.6 × 0.2vF, S, R, lbM, B * nMCG -3-60-19
NGC 776123 51 28.8-13 22 52S014.113.11.2 × 1.2F, vS, R, gbM, * 10 p 8'IC 5361, MCG -2-60-20, NPM1G -13.0659, IRAS 23488-1339
NGC 776323 50 15.7-16 35 23E-S015.314.30.7 × 0.4eF, vS, R, F * fNPM1G -16.0627
NGC 777623 54 16.5-13 35 11Sa14.813.90.9 × 0.3eF, vS, lE, gbMIC 1514, MCG -2-60-22
IC 133020 46 14.8-14 01 22Sc14.714.01.2 × 0.4F, vS, difMCG -2-53-2, IRAS 20434-1412
IC 133120 47 48.8-09 59 44S0-a14.613.71.8 × 0.6F, S, bM, rMCG -2-53-5
IC 133220 51 51.3-13 42 40Sb14.313.50.9 × 0.6F, vS, RMCG -2-53-11, NPM1G -13.0503
IC 134121 00 16.6-13 58 33S015.314.30.5 × 0.3F, vS, R, lbMMCG -2-53-16, NPM1G -14.0591
IC 134221 00 25.5-14 29 42Sc14.613.90.8 × 0.3vF, vS, E pf, lbMMCG -3-53-17, IRAS 20576-1441
IC 134421 01 16.5-13 22 49S14.513.71 × 0.4pB, pL, iF, sbMMCG -2-53-18
IC 134521 01 22.1-13 23 51E015.614.60.5 × 0.5vF, S, R, vlbMNPM1G -13.0508
IC 134621 01 37.1-13 57 37SBb14.914.11.2 × 0.6pB, vS, R, gbMMCG -2-53-19
IC 134721 01 44.3-13 18 46S015.314.40.8 × 0.6pB, RMCG -2-53-20, NPM1G -13.0510
IC 134821 01 43.9-13 21 25S015.314.30.8 × 0.4F, vS, R, bMNPM1G -13.0509
IC 134921 01 50.4-13 15 54S15.514.70.6 × 0.3vF, vS, R, lbMNPM1G -13.0511
IC 135121 01 52.3-13 12 05S015.714.70.5 × 0.2F, vS, R, lbMNPM1G -13.0512
IC 135221 01 54.8-13 23 04S16.515.70.3 × 0.1pB
IC 135321 01 56.3-13 16 21S16.515.70.3 × 0.2vF, vS, R
IC 135421 01 52.2-13 51 08S16.015.20.7 × 0.4F, vS, R, bMIC 1350, MCG -2-53-21, NPM1G -14.0595
IC 135521 01 58.3-13 10 21E015.314.30.4 × 0.4F, vS, R, bMNPM1G -13.0513
IC 135721 05 57.2-10 42 57Sa15.214.31.3 × 0.7vF, vS, iF, vlbMNPM1G -10.0600
IC 136221 11 52.6+02 19 46E?15.614.60.3 × 0.2vF, vS, R, * 14 nfCGCG 375-7, KARA 898, NPM1G +02.0485
IC 136621 14 07.9+01 46 36S15.314.50.4 × 0.2F, S, iR, bet 2 st 11 & 13CGCG 375-17, NPM1G +01.0513
IC 136821 14 12.6+02 10 42Sa14.313.41.2 × 0.4eeF, S, R, v difficUGC 11703, MCG 0-54-8, CGCG 375-18, IRAS 21116+0158
IC 137021 15 14.3+02 11 325C15.114.61.6 × 0.5vF, 2 F st invCGCG 375-21, 2ZW 111
IC 137121 20 15.6-04 52 34E-S014.813.80.9 × 0.7F, S, dif, gbM, rMCG -1-54-13, NPM1G -05.0598
IC 137221 20 17.1-05 36 17S15.514.70.8 × 0.4vF, vS, R, dif, * 14 sf
IC 137321 20 37.1+01 05 35S015.514.50.3 × 0.3F, vS, R, sbM, 2 others southMCG 0-54-13, CGCG 375-29, NPM1G +00.0565
IC 137421 21 02.6+01 42 49S?15.915.10.3 × 0.2vF, vS, lbMCGCG 375-31, KARA 908, NPM1G +01.0518
IC 138121 27 33.6-01 11 17SB15.414.60.8 × 0.5F, vS, R, bMMCG 0-54-16, CGCG 375-36, NPM1G -01.0541
IC 138321 27 39.5-01 06 08S15.314.50.4 × 0.2F, vS, R, stellarCGCG 375-37
IC 138421 27 53.0-01 22 07Irr15.414.70.7 × 0.5vF, vS, RMCG 0-54-17, CGCG 375-39
IC 138521 28 51.1-01 04 11SB?15.815.00.4 × 0.4pB, vS, RMCG 0-54-22, CGCG 375-42
IC 138721 29 34.4-01 21 02E315.514.50.4 × 0.3pB, vS, iFMCG 0-54-26, CGCG 375-45, ARAK 547, NPM1G -01.0544
IC 138821 29 52.1-00 37 51S15.014.20.4 × 0.2eF, vS, 2 st nfMCG 0-54-27, CGCG 375-46, ARAK 548, NPM1G -00.0561
IC 139021 32 24.9-01 51 43SBc15.514.50.7 × 0.6F, vS, R, bMMCG 0-55-4, CGCG 376-5
IC 139121 35 00.4-00 30 41E?15.714.70.2 × 0.2vF, S, difMCG 0-55-7, CGCG 376-10
IC 139721 44 02.2-04 53 04S15.314.50.7 × 0.3F, vS, stellarNPM1G -05.0614
IC 140121 46 59.5+01 42 41Sbc14.413.81.8 × 0.7pB, pS, rUGC 11810, MCG 0-55-15, CGCG 376-31, KARA 930, IRAS 21444+0128
IC 140321 50 29.0-02 42 56S16.615.80.5 × 0.3eF, S, F, * att, v difficNPM1G -02.0472
IC 140521 50 49.8+02 01 17SBab14.613.80.9 × 0.7pB, vS, R, bMUGC 11826, MCG 0-55-20, CGCG 376-37, NPM1G +01.0534
IC 140621 51 04.8+01 59 15E015.714.70.3 × 0.3F, vS, R, stellarCGCG 376-38, NPM1G +01.0535
IC 140921 53 19.5-07 29 59S16.015.20.5 × 0.3eF, S, iF
IC 141021 56 02.1-02 53 59E415.914.90.5 × 0.3pF, vSNNPM1G -03.0616
IC 141121 56 00.5-01 31 00E414.413.40.9 × 0.5F, vS, R, vlbMUGC 11850, MCG 0-56-1, CGCG 377-1, NPM1G -01.0553
IC 1413 121 58 25.3-03 07 29S/P16.515.70.9 × 0.2F, S, stellar
IC 1413 221 58 26.8-03 06 06S16.015.20.7 × 0.2F, S, stellar
IC 141722 00 21.7-13 08 49Sb14.513.71.3 × 0.4pB, pL, part more condensedMCG -2-56-3, IRAS 21576-1323
IC 141922 02 58.8-09 55 14S16.015.20.4 × 0.2eF, slbMNPM1G -10.0646
IC 142122 03 03.9-09 58 40E315.814.80.4 × 0.3Neb * 14mMCG -2-56-9, NPM1G -10.0647
IC 143022 07 29.7-13 34 51E016.015.00.4 × 0.4F, S, vlbM, diffic
IC 143122 07 39.5-13 30 48Sa15.114.20.8 × 0.7eF, v diffic, F * npMCG -2-56-15
IC 143322 12 10.5-12 45 54P15.714.70.7 × 0.5F, S, E pf, bMMCG -2-56-21, VV 390, NPM1G -13.0565
IC 143522 13 26.1-22 05 47Sbc13.913.11 × 0.6F, SESO 601-30, MCG -4-52-25, AM 2210-222, IRAS 22106-2220
IC 143622 13 51.3-10 11 29E-S015.814.80.7 × 0.6eF, vS, R, vSNMCG -2-56-24, NPM1G -10.0652
IC 143722 15 44.9+02 03 57S0-a14.413.51.1 × 1pB, vS, R, mbMUGC 11965, MCG 0-56-16, CGCG 377-42, KARA 956
IC 143822 16 29.0-21 25 51SBa12.811.92.4 × 2.1F, biNESO 602-1, MCG -4-52-29, IRAS 22137-2140
IC 143922 16 40.2-21 29 08SBa14.613.71.3 × 0.9vF, S, vlbMESO 602-2, MCG -4-52-30
IC 144022 16 33.2-16 00 59E?14.913.91.2 × 0.3F, S, stellarMCG -3-56-13
IC 144322 19 03.6-20 56 24E213.512.50.8 × 0.7pB, S, iF, mbMESO 602-5, MCG -4-52-33
IC 144522 25 30.2-17 14 37E-S013.512.71.6 × 1.3pF, vS, gbMNESO 602-19, MCG -3-57-7
IC 144622 29 04.6-01 11 03S15.915.10.6 × 0.3vF, stellarNPM1G -01.0563
IC 144722 29 59.8-05 07 10Sb13.612.81.5 × 0.8eeF, pS, R, * 9.0 n 3'MCG -1-57-14, IRAS 22273-0522
IC 144922 35 07.0-08 45 56S15.815.00.5 × 0.4F, S, iF, bM, r
IC 145122 46 07.4-10 22 13Sc14.914.20.5 × 0.5vF, S, dif, vS, excent NMCG -2-58-2
IC 145322 46 54.4-13 26 58SBb15.114.30.7 × 0.6pB, pL, RMCG -2-58-4
IC 145622 55 18.2-12 43 55S016.015.00.7 × 0.2vF, vS
IC 1464 A23 03 11.0-08 59 19S M15.414.60.7 × 0.4F, r, D ?MCG -2-58-20, NPM1G -09.0723
IC 1464 B23 03 12.0-08 59 32S M15.714.90.5 × 0.3F, r, D ?MCG -2-58-21, NPM1G -09.0724
IC 146923 06 28.5-13 32 11E416.015.00.5 × 0.3F, S, R, F * f
IC 147123 08 45.0-12 38 21S?14.513.60.8 × 0.4pB, S, R, bMMCG -2-59-3
IC 147923 18 46.3-10 23 55E-S014.713.71.1 × 1pF, S, R, stellarMCG -2-59-10, NPM1G -10.0713
IC 148923 26 32.1-12 30 59S15.014.20.4 × 0.2F, vS, R, * 9 southMCG -2-59-16, IRAS 23239-1247
IC 149123 29 24.5-16 18 58S?15.014.10.5 × 0.3F, S, RMCG -3-59-10
IC 149423 30 46.1-12 43 27S15.915.10.5 × 0.2F, R, lbMNPM1G -13.0644
IC 149823 31 53.5-05 00 23Sa14.613.71.9 × 0.6eeF, pS, R, * 9.5 p 36s, 3' sMCG -1-60-2
IC 150523 41 37.0-03 33 53E214.713.70.9 × 0.7eeF, pS, R, 3 st f, difficMCG -1-60-20, NPM1G -03.0698
IC 150923 47 16.6-15 18 26Sc15.214.51.4 × 0.2F, S, E ns, gbMMCG -3-60-14
IC 505020 45 15.0-05 37 23Sb14.313.51.3 × 0.9F, cS, dif, vS E NMCG -1-53-5, IRAS 20426-0548
IC 508921 10 54.4-03 51 44S16.015.20.7 × 0.3eF, vS, bM, F * 30" spNPM1G -04.0559
IC 509021 11 30.6-02 01 55Sa14.413.51.2 × 0.5vF, S, R, sbMUGC 11691, MCG 0-54-3, CGCG 375-6, IRAS 21089-0214
IC 511121 28 10.9+02 28 28S?15.314.40.7 × 0.6F, S, iFMCG 0-54-21, CGCG 375-41, KARA 917
IC 512621 40 28.6-06 20 45Sb15.714.90.5 × 0.5vF, vS, R, bet 2 st 14
IC 517822 12 33.2-22 57 16SB+C?14.713.81.1 × 0.8eF, vS, 7220 p 63sESO 532-31, MCG -4-52-22
IC 521022 22 31.1-18 52 09E-S014.013.01.2 × 1.1eeF, vS, R, p of 2ESO 602-12, MCG -3-57-4
IC 521122 22 42.9-18 52 47Sab14.313.51 × 0.6eF, S, f of 2ESO 602-14, MCG -3-57-5
IC 524122 41 38.5+02 38 23SBc14.613.91 × 0.8pB, cS, R, gbM, rUGC 12152, MCG 0-57-8, CGCG 378-16, KUG 2239+023
IC 526122 54 25.2-20 21 48SBc13.913.21.5 × 1.3eeF, pL, R, v diffic, * 9 p 22sESO 603-26, MCG -4-54-1, IRAS 22517-2037
IC 527823 00 15.9-08 10 43Sd15.815.21.2 × 0.4eF (not verified)MCG -1-58-14
IC 530423 18 52.5-10 15 32E-S014.413.41.4 × 0.9eF, S, R, 3 or 4 F st spMCG -2-59-11, NPM1G -10.0714
IC 531023 20 47.7-22 08 56E015.814.80.5 × 0.5eF, eS, alm stell, * 9.5 n 5'ESO 605-1, NPM1G -22.0398
IC 532123 26 20.0-17 57 24Sa13.913.01.3 × 0.8eF, vS, R, * 10 np 1'ESO 605-7, MCG -3-59-9, IRAS 23237-1813
IC 532723 30 47.5-13 29 07Sb14.113.31.4 × 1pF, pS, * 11 f 1'IC 1495, MCG -2-59-24, IRAS 23281-1345
IC 533423 34 36.4-04 32 02Sab14.113.31.8 × 0.6Neb * 10.5 (? close D *)MCG -1-60-8
IC 534323 39 22.4-22 29 50Irr14.013.60.8 × 0.6eF, pS, * 7.5 sf 19sESO 536-15, MCG -4-55-19
IC 534523 39 32.3-22 24 48Sbc14.513.70.8 × 0.6vF, vS, R, 6' n of Sw. XI.ESO 536-16, MCG -4-55-20, IRAS 23369-2241

«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 G036.1-57.122 29 39-20 50 15NGC 729336-57.122267-2102CURTIS 1918ARO 17, VV 275, VV' 563 980. 660. 0.30 -28.2 ± 3.0 14.0 (O-III), 24. (N-II)AG82 441, CSI -21 -22270, GCRV 14134, PLX 5437, USNO 271, WD 2201 -21. 1U: 11.81, B: 13.10, V: 13.50Hg O(H)
PN G037.7-34.521 04 11-11 21 57NGC 700937-34.121014-1133HERSCHEL 1782ARO 16, VV 259, VV' 541, EM* CDS 1211 28.5 0.60 -44.0 ± 3.0 20.6 (O-III), 20.0 (N-II)AG82 419, BD -11 5511, GCRV 13233, HD 200516, TD1 27614B: 12.66, V: 12.78O(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)
NGC 6981M 7220 53 27.70-12 32 14.317.012.9-1.4240.0516.9016.319.27-7.040.140.720.450.94F70.02-345.0 ± 3.7-336.21.21 0.460.9319.022.388.729.23
NGC 7089M 221 33 27.02-00 49 23.711.510.4-1.6550.0616.0515.506.47-9.030.090.660.460.92F40.11-5.3 ± 2.03.88.2 ± 0.61.59 0.321.0615.784.008.489.40
NGC 749223 08 26.63-15 36 41.426.325.3-1.7850.0017.6317.1011.29-5.810.230.420.24-177.5 ± 0.6-176.21.2 ± 1.00.72 0.861.1520.681.279.609.44

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