Constellation Aquarius (Water Bearer)

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 Name	Aquarius
IAU Genitive	Aquarii
IAU Abbr.	Aqr
English Name	Water Bearer
Season (47° N)	July … December
Right Ascension	20^h 38^m 19^s … 23^h 56^m 27^s
Declination	-24° 54' 15" … +03° 19' 32"
Area	980 deg²
Neighbours (N↻)	Peg, Equ, Del, Aql, Cap, PsA, Scl, Cet, Psc

Deep-Sky Object Descriptions

Messier 2

Messier 72

Messier 73

Saturn Nebula
NGC 7009

Helix Nebula
NGC 7293

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.

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 7890			BD-02 5328	196712	144666						20 39 13.2	-02 24 46	6.22	B7IIIne v			VAR:H alpha varies.
HR 7897		1	BD-00 4064	196758	126062	3651	I		14108		20 39 24.9	+00 29 11	5.16	K1III	7.1	59.7	D:Both companions optical.
HR 7946			BD-03 5018	197954	144802		I				20 47 03.6	-02 29 12	6.27	K2
HR 7950	ε	2	BD-10 5506	198001	144810	781					20 47 40.6	-09 29 45	3.77	A1V			N:Albali; Al Bali.
HR 7951		3	BD-05 5378	198026	144814	1543	I			EN Aqr	20 47 44.2	-05 01 40	4.42	M3III			VAR:Lb 4.41 - 4.45V.
HR 7976			BD-13 5773	198431	163924	3665					20 50 41.8	-12 32 42	5.88	gK1
HR 7982		4	BD-06 5604	198571	144877				14360	13350	20 51 25.7	-05 37 35	5.99	F5V+F7V	0.9	1.1	D:AB 6.4 F5V, 7.22 F8V, 187y, a = 0.855". Mag., colors for combined light.,DYN:0.019".
HR 7985		5	BD-06 5606	198667	144889					13360	20 52 08.7	-05 30 25	5.55	B9III
HR 7990	μ	6	BD-09 5598	198743	144895	1547		S			20 52 39.2	-08 59 00	4.73	A3m			SB:1782d, K 5.4k/s, V0 -11.4k/s, asini 128.
HR 7994			BD-12 5854	198802	163953			S			20 53 05.6	-11 34 25	6.38	G1V		0.2
HR 7998			BD-07 5433	198949	144915						20 53 58.4	-06 53 23	6.44	F1IV
HR 8006			BD-01 4075	199124	144941					EM Aqr	20 55 08.1	-01 22 24	6.55	A9Vn			VAR:Delta Sct 6.55 - 6.58V, 0.054d. Per. and amp. may vary.
HR 8014			BD-04 5307	199280	144957						20 56 18.3	-03 33 41	6.57	B8Vn
HR 8015		7	BD-10 5553	199345	144968		I		14449	13419	20 56 54.0	-09 41 51	5.51	gK5	3.5	176.6	D:AB fixed sep. B, 11.8v at 36".
HR 8017			BD-00 4132	199442	126396				14457		20 57 10.6	+00 27 49	6.05	K2III	5.4	26.2	D:AB, CPM.
HR 8024			BD-15 5848	199603	164027					DV Aqr	20 58 41.9	-14 28 58	6.01	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 8041		11	BD-05 5433	199960	145022	789					21 00 33.8	-04 43 49	6.21	G1V
HR 8054			BD-01 4095	200340	145050						21 02 59.6	-00 55 29	6.50	B6V
HR 8056			BD+00 4648	200375	126491				14573		21 03 03.0	+01 31 55	6.25	F5V	0.5	1.3	D:AB 6.74 F5, 7.21, 3055y, a = 3.740".,DYN:0.015".
HR 8058		12	BD-06 5664	200496	145064				14592		21 04 04.6	-05 49 24	7.31 H	A3V	1.9	2.7	D:CPM with HR 8059.
HR 8059		12	BD-06 5664	200497	145065				14592		21 04 04.7	-05 49 23	5.89 H	G4III	1.9	2.7	D: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 8068			BD+01 4418	200663	126522	3681					21 04 45.4	+02 16 11	6.33	G5
HR 8093	ν	13	BD-11 5538	201381	164182	794	I				21 09 35.7	-11 22 18	4.51	G8III
HR 8096			BD-09 5674	201567	145171						21 10 46.9	-09 21 14	6.27	K0III
HR 8102			BD-15 5908	201707	164204					EW Aqr	21 11 41.3	-14 28 20	6.48	F0Del Del:			G:Hyades group.,S:Also classified F0III-IV.,VAR:Delta Sct 6.41 - 6.48V, 0.097d.
HR 8118			BD-11 5553	202149	164240						21 14 16.7	-10 36 19	6.77	B9pHgMn
HR 8121			BD-00 4186	202259	145229		I			13614	21 14 37.0	+00 05 32	6.38	M1III			VAR:Amp. 0.045V.
HR 8132			BD-02 5495	202554	145259						21 16 39.6	-01 36 28	6.48	K0
HR 8134			BD-13 5897	202606	164279						21 17 13.5	-13 16 44	6.40	A2V
HR 8141		15	BD-05 5512	202753	145278	3698					21 18 11.1	-04 31 10	5.82	B5V			M:Old disk population runaway star.
HR 8160		16	BD-05 5524	203222	145317						21 21 04.3	-04 33 36	5.87	gG7
HR 8175		17	BD-09 5728	203525	145351	3705	I				21 22 56.3	-09 19 10	5.99	M0III
HR 8187		18	BD-13 5923	203705	164364	1562		W		13684	21 24 11.5	-12 52 41	5.49	F1V	7.5	48.9
HR 8192		20	BD-04 5444	203843	145376						21 24 51.7	-03 23 54	6.36	F0III
HR 8195		19	BD-10 5668	203875	145382						21 25 13.1	-09 44 55	5.70	F0IV
HR 8199		21	BD-04 5446	203926	145384	3708	I				21 25 17.0	-03 33 24	5.49	K4III
HR 8203			BD-00 4215	204041	126789						21 25 51.5	+00 32 04	6.46	A1IV
HR 8205			BD+00 4726	204121	126794	3711					21 26 28.1	+01 06 12	6.13	F5V
HR 8232	β	22	BD-06 5770	204867	145457	808	I		15050		21 31 33.5	-05 34 16	2.91	G0Ib	7.9	35.5	D: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 8251			BD-04 5489	205423	145510						21 35 17.6	-03 58 59	5.77	gG9
HR 8263			BD-01 4180	205765	145533				15142		21 37 33.8	-00 23 25	6.25	A2V	3.3	31.5	D:CPM.,G:UMa stream.
HR 8264	ξ	23	BD-08 5701	205767	145537	1569		S			21 37 45.1	-07 51 15	4.69	A7V	2.0	0.1	D: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 8277		25	BD+01 4517	206067	126965	3729	I	W			21 39 33.3	+02 14 37	5.10	K0III	6.3	136.8
HR 8287		26	BD+00 4770	206445	126997		I				21 42 10.1	+01 17 07	5.67	K2III			G:In Ursa cluster?
HR 8332			BD-06 5827	207235	145671						21 47 38.1	-05 55 02	6.17	A7V
HR 8360			BD-04 5568	208111	145731						21 54 10.4	-04 16 34	5.71	K2III
HR 8363			BD-03 5329	208177	145735				15432		21 54 35.9	-03 18 04	6.20	F5IV	3.4	17.6	D:Optical.
HR 8376			BD-06 5878	208703	145778						21 58 13.3	-05 25 29	6.33	F5IV
HR 8382			BD-05 5674	208801	145784	1580					21 58 55.0	-04 22 23	6.22	K2V
HR 8390		28	BD-00 4296	209128	127235		I				22 01 05.0	+00 36 18	5.58	gK4
HR 8394			BD-18 6056	209240	164827	3761					22 02 11.9	-17 54 13	6.28	gG7
HR 8396		29	BD-17 6422	209278	164830				15562 A	DX Aqr	22 02 26.6	-16 57 51	6.37	A2V+K0III	0.1	3.6	D: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 8401		30	BD-07 5688	209396	145836						22 03 16.4	-06 31 21	5.54	K0III
HR 8402	ο	31	BD-02 5681	209409	145837	3765				Omi Aqr	22 03 18.9	-02 09 19	4.69	B7IVe			S:Shell star.,VAR:Gamma Cas 4.68 - 4.89V, 4.57 - 4.65p.
HR 8410		32	BD-01 4242	209625	145853						22 04 47.4	-00 54 24	5.30	A5m v			G: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 8414	α	34	BD-01 4246	209750	145862	827	I	W			22 05 47.0	-00 19 11	2.96	G2Ib v	9.0	113.0	G:See HR 8232.,N:SADALMELIK; Sadalmelek; Sadlamulk; El Melik; Saad el Melik.,VAR:He 10830 possibly variable.
HR 8418	ι	33	BD-14 6209	209819	164861	828					22 06 26.2	-13 52 11	4.27	B9IV-V
HR 8439		35	BD-19 6227	210191	164888						22 08 59.0	-18 31 11	5.81	B2.5IV
HR 8451			BD-04 5623	210419	145914						22 10 21.1	-03 53 39	6.27	A1Vnn
HR 8452		38	BD-12 6196	210424	164910	3771					22 10 37.5	-11 33 54	5.46	B7III
HR 8453			BD-04 5625	210434	145916						22 10 33.8	-04 16 02	6.01	K0III-IV
HR 8457			BD-21 6173	210464	190945						22 11 02.4	-21 13 57	6.09	F6V
HR 8462		39	BD-14 6229	210705	164923					14068	22 12 25.8	-14 11 38	6.03	F2V
HR 8467			BD-05 5732	210763	145940						22 12 43.8	-04 43 15	6.39	F7V
HR 8480		41	BD-21 6180	210960	190986				15753		22 14 18.0	-21 04 27	5.32	K0III+F2V	1.6	5.1	D:AB binary. B is F8V.,DYN:0.011".
HR 8495			BD-02 5726	211356	145989						22 16 33.6	-01 35 47	6.15	A5Vn
HR 8496		42	BD-13 6148	211361	164974		I				22 16 48.1	-12 49 53	5.34	gK0
HR 8497			CD-2317344	211364	191021						22 16 59.8	-23 08 24	6.17	G5
HR 8499	θ	43	BD-08 5845	211391	145991	840	I				22 16 50.0	-07 47 00	4.16	G8III-IV			N:Ancha.
HR 8500			BD-09 5948	211392	145992					14095	22 16 52.6	-09 02 24	5.79	gK3
HR 8504		44	BD-06 5960	211434	145993	3782				14100	22 17 06.5	-05 23 14	5.75	G6III
HR 8507			BD-00 4333	211575	146004			S			22 18 04.3	-00 14 16	6.39	F3V		0.1
HR 8508		45	BD-14 6255	211676	164996						22 19 00.8	-13 18 18	5.95	gG7
HR 8512	ρ	46	BD-08 5855	211838	146023						22 20 11.9	-07 49 16	5.37	B8IIIpMn:Hg:
HR 8516		47	BD-22 5897	212010	191083	1584	I				22 21 35.6	-21 35 54	5.13	K2III
HR 8518	γ	48	BD-02 5741	212061	146044	842			15864	14132	22 21 39.4	-01 23 14	3.84	A0V	7.9	37.4	D:Optical.,N:Sadalachbia; Sadachbia.,S:Lambda Boo star.,SB:ADS 15864A. Unresolved by speckle interferometry.
HR 8529		49	CD-2515905	212271	191105						22 23 30.9	-24 45 45	5.53	gG9
HR 8530			BD-07 5765	212320	146062			D			22 23 32.1	-07 11 40	5.93	G6IIIBaII			D:Suspected occultation double. Unresolved by speckle interferometry.
HR 8533		51	BD-05 5780	212404	146067				15902		22 24 06.9	-04 50 13	5.78	A0V	0.0	0.3	D:AB 6.6 A0, 6.6, 190y, a = 0.490". Measured sep. 0.121" on 1985.5 by speckle interferometry.
HR 8534		50	BD-14 6276	212430	165044	3791					22 24 27.1	-13 31 46	5.76	G6.5III
HR 8539	π	52	BD+00 4872	212571	127520	1585	I			Pi Aqr	22 25 16.6	+01 22 39	4.66	B1Ve v			RV: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 8542			CD-2417171	212643	191144	3793					22 26 10.7	-23 40 57	6.29	A0V
HR 8544		53	BD-17 6520	212697	165077				15934 B		22 26 34.2	-16 44 29	6.57 H	G2V	0.2	3.3	D:Binary with HR 8545. Components C, D, optical.,DYN:0.083".
HR 8545		53	BD-17 6521	212698	165078				15934 A		22 26 34.4	-16 44 33	6.35 H	G1V	0.2	3.3	D:See HR 8544. Colors for combined light. Mag. of blend 5.56V.,DYN:0.083".
HR 8558	ζ¹	55	BD-00 4365	213051	146107		I		15971 B		22 28 49.7	-00 01 13	4.59 H	F6IV	0.2	1.8	D: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 8559	ζ²	55	BD-00 4365	213052	146108		I		15971 A		22 28 50.1	-00 01 12	4.42 H	F3V	0.2	1.8	D: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 8565			BD-13 6204	213198	165123						22 30 01.5	-12 54 54	6.40	F3IV			G:Hyades group.
HR 8567		56	BD-15 6231	213236	165127						22 30 17.4	-14 35 09	6.37	B8V s			S:Hg, Mn. May resemble HR 1339 (53 tau).
HR 8573	σ	57	BD-11 5850	213320	165134	1591					22 30 38.8	-10 40 41	4.82	A0IV s			G:In Ursa cluster?
HR 8580			BD-03 5460	213428	146136	3802					22 31 18.4	-02 54 40	6.16	K0
HR 8581			BD-07 5797	213429	146135			S			22 31 18.4	-06 33 18	6.14	F7V		0.1
HR 8583		58	BD-11 5855	213464	165147						22 31 41.3	-10 54 20	6.38	A8III
HR 8590		60	BD-02 5781	213789	146160			W			22 34 02.9	-01 34 27	5.89	G6III	4.4	98.1
HR 8592	υ	59	BD-21 6251	213845	191235	849					22 34 41.6	-20 42 30	5.20	F4IV
HR 8596			CD-2417232	213986	191246						22 35 36.5	-23 59 28	5.97	gK0
HR 8597	η	62	BD-00 4384	213998	146181	850					22 35 21.4	-00 07 03	4.02	B9IV-Vn
HR 8610	κ	63	BD-04 5716	214376	146210	1595	I	W			22 37 45.4	-04 13 41	5.03	K2III	3.5	98.3	N:Situla.,R:Occultation diameter = 0.0035".
HR 8612			BD-08 5912	214448	146216				16130	14255	22 38 22.2	-07 53 52	6.23	G0III+F0V	1.8	0.2	D: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 8629			BD-04 5728	214810	146239			W			22 40 48.0	-03 33 15	6.31	F6V	0.5	0.3	D: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 8645			BD-09 6038	215114	146271				16208		22 43 03.5	-08 18 42	6.45	A5V	1.1	2.5	D:AB binary. B9, A7.
HR 8647		67	BD-07 5838	215143	146273	3819					22 43 14.3	-06 57 46	6.41	A0Vn
HR 8649		66	BD-19 6324	215167	165252		I			14291	22 43 35.3	-18 49 49	4.69	K4III			G:UMa stream.
HR 8670		68	BD-20 6486	215721	165293	1597	I				22 47 33.1	-19 36 48	5.26	G7III
HR 8673	τ¹	69	BD-14 6346	215766	165298				16268		22 47 42.8	-14 03 23	5.66	A0V	3.9	23.7	D:AB optical.,N:Sometimes called Tau1 Aqr; usually no Greek letter. See HR 8679.
HR 8676		70	BD-11 5923	215874	165308	3825				FM Aqr	22 48 30.2	-10 33 20	6.19	A9III-IV			VAR:Delta Sct 6.16 - 6.19V, 0.087d.
HR 8679	τ²	71	BD-14 6354	216032	165321	861	I	W		14329	22 49 35.5	-13 35 33	4.01	M0III	4.5	132.5	N:Sometimes called Tau2 Aqr; usually without superscript.
HR 8698	λ	73	BD-08 5968	216386	146362	864	I			Lam Aqr	22 52 36.9	-07 34 47	3.74	M2.5IIIaFe-1 e			R:Occultation diam. = 0.0074".,S:Ultraviolet FeII emission.,VAR:Lb 3.70 - 3.80V.
HR 8704		74	BD-12 6371	216494	165359			S		HI Aqr	22 53 28.7	-11 37 00	5.80	B9III	0.5	0.1	D: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 8709	δ	76	BD-16 6173	216627	165375	866				14356	22 54 39.0	-15 49 15	3.27	A3V			G:Sirius group. Possible Eggen group with HR 63, q.v.,N:Skat; Scheat; Sheat.,S:Also classified A2-4III.
HR 8710		78	BD-07 5886	216637	146382						22 54 34.1	-07 12 17	6.19	K3III
HR 8711		77	BD-17 6619	216640	165376					14358	22 54 45.5	-16 16 19	5.56	K2.5IIIb
HR 8716			BD-05 5885	216718	146388				16365	14360	22 55 11.0	-04 59 16	5.72	K0III-IV	2.0	0.6	D:120.0y, e 0.68, a 0.47", i 85d, mag. diff 2.0.,VAR:ADS 16365B, 7.6v.
HR 8727			BD-05 5894	216953	146404						22 57 17.2	-04 48 36	6.31	G9III
HR 8741			BD-13 6318	217251	165425		I				22 59 35.7	-13 04 15	6.07	K5III
HR 8756			CD-2317706	217498	191585	3842					23 01 23.0	-22 47 27	6.28	A5V
HR 8757		81	BD-07 5910	217531	146447		I				23 01 23.6	-07 03 40	6.21	K5III
HR 8759			BD-05 5910	217563	146451			D			23 01 31.7	-04 42 41	5.94	K0			D:Suspected occultation double.
HR 8763		82	BD-07 5913	217701	146465		I				23 02 32.6	-06 34 27	6.15	M2III			G:Wolf 630 group.
HR 8764			BD-21 6354	217703	191604						23 02 44.3	-20 52 14	5.97	K0III-IV
HR 8772			BD-05 5917	217877	146482						23 03 57.3	-04 47 43	6.68	F8V			G:Hyades group.
HR 8782		83	BD-08 6018	218060	146498				16497		23 05 09.8	-07 41 37	5.43	F2IV+F0V	0.2	0.2	D: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 8783			BD-17 6661	218061	165481	3846	I	W			23 05 12.8	-17 04 45	6.14	K0	5.1	56.1
HR 8789		86	CD-2417497	218240	191651		I		16511		23 06 40.9	-23 44 35	4.47	G9III	10.0	2.9	D:Sep. 2.9" observed 1925; single in 1929.
HR 8812		88	BD-21 6368	218594	191683	873	I				23 09 26.8	-21 10 21	3.66	K1III
HR 8816			BD-15 6360	218639	165522	3856					23 09 49.6	-14 30 38	6.42	A0Vn
HR 8817		89	CD-2317771	218640	191687		I	W			23 09 54.8	-22 27 27	4.69	G2IV+A2V	0.8	0.4	S:Also classified G2III + A2V.
HR 8834	φ	90	BD-06 6170	219215	146585	1607	I				23 14 19.4	-06 02 56	4.22	M1.5III			G:Arcturus group.,R:Occultation diam. = 0.0049".
HR 8836			BD-11 6032	219279	165578		I		16618		23 14 40.2	-10 41 19	6.12	K5III	4.5	3.5	D:AB, CPM.
HR 8840			BD-04 5852	219402	146593	3860					23 15 34.3	-03 29 47	5.55	A3V
HR 8841	ψ¹	91	BD-09 6156	219449	146598	1608	I		16633 A		23 15 53.5	-09 05 16	4.21	K0III	4.8	49.2	D: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 8850	χ	92	BD-08 6076	219576	146612		I			Chi Aqr	23 16 50.9	-07 43 36	5.06	M3III			VAR:Lb 4.9 - 5.25V, 6.5 - 6.8p.
HR 8856			BD-12 6461	219659	165609					14483	23 17 40.0	-11 42 47	6.34	A1Vn
HR 8858	ψ²	93	BD-09 6160	219688	146620			D			23 17 54.2	-09 10 57	4.39	B5V			D:Suspected occultation double.
HR 8865	ψ³	95	BD-10 6094	219832	146635	1609			16671	14491	23 18 57.7	-09 36 39	4.98	A0V	3.9	1.4	D:AB binary.,G:Hyades group.,VAR:ADS 16671B, 9.0 - >12?v.
HR 8866		94	BD-14 6448	219834	165625				16672 A		23 19 06.7	-13 27 32	5.08	G5IV	2.4	0.2	D: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 8868		96	BD-05 5966	219877	146639				16676		23 19 24.0	-05 07 28	5.55	F3IV-V	4.9	10.6	D:CPM.,G:Hyades moving group.
HR 8869			BD-18 6283	219879	165628	3868	I				23 19 24.1	-18 04 31	5.93	gK3
HR 8879			BD-06 6191	220035	146652			D		14515	23 20 40.9	-05 54 29	6.17	K0III			D:Suspected occultation double.
HR 8890		97	BD-15 6406	220278	165658				16708		23 22 39.2	-15 02 21	5.20	A3Vp	0.7	0.4	D: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 8892		98	BD-20 6587	220321	191858	1612	I				23 22 58.2	-20 06 02	3.97	K0III
HR 8900			BD-19 6450	220465	165672						23 24 07.8	-18 41 15	6.19	G8III
HR 8906		99	BD-21 6420	220704	191900		I			14554	23 26 02.8	-20 38 31	4.39	K5III			G:Sirius group.
HR 8917			BD-12 6496	220957	165708						23 28 05.2	-11 26 59	6.37	G0V
HR 8921			BD-10 6120	221081	146729		I				23 29 00.6	-09 15 58	6.18	K0
HR 8924			BD-05 5999	221148	146736	3881				14588	23 29 32.1	-04 31 58	6.25	K3III v
HR 8928			BD-07 6036	221308	146748						23 31 01.1	-06 17 18	6.39	K0
HR 8931			BD-04 5896	221356	146752						23 31 31.5	-04 05 14	6.49	F8V
HR 8932		100	BD-22 6141	221357	191970	3885					23 31 42.1	-21 22 10	6.29	A9III
HR 8939		101	BD-21 6437	221565	191988			W			23 33 16.6	-20 54 52	4.71	A1n	2.3	1.0
HR 8946			BD-16 6314	221745	165780		I				23 34 49.4	-15 14 45	5.96	K0
HR 8951			BD-08 6142	221835	146795	888					23 35 32.1	-07 27 52	6.39	gG5
HR 8958			BD-13 6439	222093	165804				16878		23 37 39.6	-13 03 37	5.65	G9IIIFe-0.5	3.9	31.6
HR 8968	ω¹	102	BD-15 6471	222345	165818						23 39 47.1	-14 13 18	5.00	F0IV
HR 8978			CD-2417796	222485	192083		I			14665	23 41 07.0	-24 09 37	6.60	M1III			VAR:Amp. 0.05(B-V).
HR 8979			BD-12 6535	222493	165828						23 41 08.9	-11 40 50	5.89	G9III			G:Probable Hyades group
HR 8980		103	BD-18 6357	222547	165834		I				23 41 34.5	-18 01 38	5.34	K5III
HR 8982		104	BD-18 6358	222574	165836		I	W		14671	23 41 45.8	-17 48 59	4.82	G0Ib-II	2.8	120.1
HR 8987			BD-16 6345	222643	165841		I				23 42 27.9	-15 26 52	5.28	K4III			SB:Unresolved by speckle interferometry 1986.45.
HR 8988	ω²	105	BD-15 6476	222661	165842	894			16944		23 42 43.3	-14 32 42	4.49	B9.5V	6.0	5.0	D:Component B, CPM, A5Vep; however, the companion is optical.
HR 8992			BD-16 6352	222800	165849		I			R Aqr	23 43 49.5	-15 17 04	6.36	M7IIIpe v			S: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 8998		106	BD-19 6500	222847	165854	1621					23 44 12.1	-18 16 37	5.24	B9Vn
HR 9002		107	BD-19 6506	223024	165867				16979 A		23 46 00.9	-18 40 41	5.29	F2III+F2V	1.0	6.6	D:11813y, a = 14.21". Companion F2III or F2V, sources discordant; vsini 96k/s.,DYN:0.027".
HR 9009			BD-12 6559	223170	165880						23 47 15.9	-11 54 39	5.73	gK1
HR 9014			BD-07 6086	223311	146919	3912	I			14715	23 48 32.5	-06 22 50	6.07	K4III
HR 9021			BD-16 6373	223428	165905						23 49 31.6	-15 51 40	6.24	K2IIIbFe-0.5
HR 9027			BD-10 6177	223524	165911	897					23 50 14.7	-09 58 27	5.94	K0IV
HR 9029			BD-15 6507	223559	165915						23 50 33.3	-14 24 07	5.72	K4.5IIIb
HR 9031		108	BD-19 6522	223640	165918					ET Aqr	23 51 21.3	-18 54 32	5.18	B9pSiSrCr v			RV: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 9037			BD-15 6515	223774	165933						23 52 30.0	-14 15 04	5.87	K3III
HR 9040			BD-09 6277	223807	146953						23 52 50.5	-08 59 48	5.75	K0III
HR 9043			CD-2417897	223884	192218						23 53 20.8	-24 13 45	6.24	A3Shell			S:Weak shell absorption; no emission.

Revised+Historic NGC/IC, Version 22/9, © Dr. Wolfgang Steinicke ^[277]
Planetary Nebulae
Name	RA	Dec	Type	bMag	vMag	Dim	Dreyer Description	Identification, Remarks
NGC 7009	21 04 10.8	-11 21 47	PN	8.3	8.0	0.58	!!!, planetary, vB, S, elliptic	PK 37-34.1, CS=11.5, Saturn nebula
NGC 7293	22 29 38.4	-20 50 11	PN	7.5	7.3	17.57	! pF, vL, E or biN (Auw 48)	PK 36-57.1, ESO 602-PN22, CS=13.5, Helix nebula
Globular Clusters
Name	RA	Dec	Type	bMag	vMag	Dim	Dreyer Description	Identification, Remarks
NGC 6981	20 53 27.9	-12 32 11	IX		9.2	6.6	globular, pB, pL, R, gmCM, rrr	M 72, GCL 118
NGC 7089	21 33 27.2	-00 49 22	II		6.6	16	!!, globular, B, vL, gpmbM, rrr, st eS	M 2, GCL 121
NGC 7492	23 08 26.7	-15 36 39	XII		11.2	4.2	eF, L, bet 2 D st	GCL 125
Galaxies
Name	RA	Dec	Type	bMag	vMag	Dim	Dreyer Description	Identification, Remarks
NGC 6945	20 39 00.5	-04 58 20	E-S0	14.4	13.4	1.6 × 0.8	pF, vS, R, mbM	MCG -1-52-15, near SAO 144663
NGC 6959	20 47 07.2	+00 25 49	S0	14.7	13.7	0.6 × 0.3	vF	CGCG 374-13
NGC 6961	20 47 10.4	+00 21 50	E2	14.7	13.7	0.6 × 0.5	eF, vS	CGCG 374-14, NPM1G +00.0554
NGC 6962	20 47 18.9	+00 19 19	SBab	13.0	12.1	2.9 × 2.2	cF, S, R, bM	UGC 11628, MCG 0-53-3, CGCG 374-15, KCPG 548A, IRAS 20447+0008
NGC 6964	20 47 24.2	+00 18 05	E2	14.0	13.0	1.7 × 1.3	F, vS, R, bM, * 14 sf ½'	UGC 11629, MCG 0-53-5, CGCG 374-17, KCPG 548B
NGC 6965	20 47 20.5	+00 29 03	S0	15.0	14.0	0.6 × 0.4	vF, vS	IC 5058, MCG 0-53-4, CGCG 374-16
NGC 6967	20 47 34.0	+00 24 44	S0-a	14.0	13.1	0.9 × 0.6	eF, vS, * 10 50" f	UGC 11630, MCG 0-53-6, CGCG 374-18, IRAS 20450+0013
NGC 6968	20 48 32.4	-08 21 35	E-S0	14.3	13.3	1.5 × 1.1	F, S, R, gbM, F * inv	MCG -2-53-6, NPM1G -08.0539, IRAS 20458-0829
NGC 6976	20 52 25.9	-05 46 17	Sbc	14.8	14.0	0.8 × 0.7	eF, iR	NGC 6975, MCG -1-53-15, NPM1G -05.0582, HCG 88C
NGC 6977	20 52 29.6	-05 44 45	SBb	14.1	13.2	1.3 × 0.9	vF, S, iR	MCG -1-53-16, HCG 88B, NPM1G -05.0583, IRAS 20499-0555
NGC 6978	20 52 35.4	-05 42 40	Sb	14.1	13.3	1.5 × 0.7	vF	MCG -1-53-17, HCG 88A, IRAS 20499-0554
NGC 6985	20 45 03.0	-11 06 15	Sa	14.7	13.8	1.5 × 0.8	eF, vS, iR	MCG -2-53-1, VV 546, IRAS 20422-1117
NGC 6985 A	20 45 01.4	-11 06 29	S	15.5	14.7	0.5 × 0.3	eF, vS, iR	MCG -2-53-1, VV 546
NGC 7001	21 01 07.7	-00 11 41	Sab	13.7	12.9	1.4 × 1.1	eF, S, E 0°	UGC 11663, MCG 0-53-16, CGCG 374-37, NPM1G -00.0540, IRAS 20585-0023
NGC 7010	21 04 39.4	-12 20 16	E5	14.0	13.0	1.9 × 1	eF, pL, R, r	IC 5082, MCG -2-53-24, NPM1G -12.0537
NGC 7047	21 16 27.4	-00 49 35	SBb	14.2	13.4	1.2 × 0.7	eF, vS, biN pf	UGC 11712, MCG 0-54-10, CGCG 375-23, IRAS 21138-0102
NGC 7051	21 19 51.3	-08 46 57	Sa	13.9	13.0	1.4 × 1.1	vF, R, gbM, ** nr	MCG -2-54-4, IRAS 21171-0859
NGC 7065	21 26 42.2	-06 59 41	SBab	14.2	13.4	1.1 × 0.9	vF, sbM, (m has 19m 33s)	MCG -1-54-17, NPM1G -07.0504
NGC 7065 A	21 26 57.8	-07 01 16	SBc	14.0	13.1	1 × 0.9	vF, sbM, (m has 19m 33s)	MCG -1-54-18, NPM1G -07.0505, IRAS 21242-0714
NGC 7069	21 28 05.8	-01 38 47	E-S0	14.4	13.4	1.3 × 0.8	vF, S, R, stell	UGC 11747, MCG 0-54-19, CGCG 375-40
NGC 7077	21 29 59.5	+02 24 53	E1	14.1	13.1	0.8 × 0.7	F	UGC 11755, MCG 0-54-28, MK 900, CGCG 375-47, ARAK 549, NPM1G +02.0497
NGC 7081	21 31 24.3	+02 29 28	Sb	13.5	12.7	1.3 × 1.3	F, S, R, mbM, * 14 s	UGC 11759, MCG 0-54-30, CGCG 375-49, KAZ 526, IRAS 21288+0216
NGC 7108	21 41 53.7	-06 42 31	E?	15.1	14.1	1.4 × 0.9	vF, S, R, stell	NGC 7111, MCG -1-55-2
NGC 7120	21 44 33.2	-06 31 23	Sb	14.8	14.0	0.8 × 0.4	vF, S, vlE	MCG -1-55-6, IRAS 21419-0645
NGC 7121	21 44 52.6	-03 37 11	Sbc	14.2	13.4	1.1 × 0.6	vF, vS, R, vlbM	MCG -1-55-8, IRAS 21422-0351
NGC 7164	21 56 23.5	+01 21 52	S0-a	15.1	14.2	0.7 × 0.5	eF, R, 4 vF st n	CGCG 377-6, NPM1G +01.0536
NGC 7165	21 59 26.1	-16 30 46	Sab	14.5	13.7	0.9 × 0.8	eF	MCG -3-56-2, IRAS 21567-1645
NGC 7167	22 00 30.8	-24 37 59	SBc	13.2	12.5	1.7 × 1.3	F, pS, R, vglbM, * 10 f	ESO 532-9, MCG -4-52-1, AM 2157-245, IRAS 21576-2452
NGC 7170	22 01 26.3	-05 25 56	E-S0	14.8	13.8	1.2 × 0.8	vF, pS, iR, bMN, D * p 36 s
NGC 7171	22 01 01.9	-13 16 11	SBb	12.9	12.2	2.6 × 1.5	vF, cL, E 124°, vgbM	MCG -2-56-5, IRAS 21583-1330
NGC 7180	22 02 18.5	-20 32 52	S0	13.6	12.6	1.5 × 0.7	vF, S, R, lbM, p of 2	ESO 601-6, MCG -4-52-8
NGC 7181	22 01 43.4	-01 57 36	S0	15.0	14.0	1 × 0.8	eF, vS, stellar	CGCG 377-14, NPM1G -02.0476
NGC 7182	22 01 51.6	-02 11 46	S0-a	15.3	14.4	0.9 × 0.4	eF, vS, stellar	MCG 0-56-6, CGCG 377-15, NPM1G -02.0477
NGC 7183	22 02 21.2	-18 54 56	S0-a	12.9	12.0	3.8 × 1.1	vF, pL, E 90°, lbM	ESO 601-8, MCG -3-56-4, IRAS 21596-1909
NGC 7184	22 02 39.9	-20 48 45	SBc	11.7	10.9	5.9 × 1.3	pB, pL, mE 64°, bet 3 st, er	ESO 601-9, MCG -4-52-9, UGCA 425, IRAS 21599-2103
NGC 7185	22 02 56.6	-20 28 17	E/SB0	13.4	12.6	2.3 × 1.5	vF, pL, iR, vglbM, f of 2	ESO 601-10, MCG -4-52-11
NGC 7188	22 03 29.0	-20 19 03	SBbc	14.0	13.2	1.6 × 0.8	eF, pS, E, lbM	ESO 601-11, MCG -4-52-12
NGC 7189	22 03 15.9	+00 34 17	SBb	14.3	13.5	1 × 0.7	F, S, lE	UGC 11882, MCG 0-56-7, CGCG 377-17, IRAS 22007+0019
NGC 7198	22 05 14.1	-00 38 52	S0/P	14.3	13.3	1.5 × 1	eF, vS, stellar	MCG 0-56-8, CGCG 377-23, NPM1G -00.0573
NGC 7211	22 06 21.8	-08 05 22	S0	15.3	14.3	1 × 0.7	eF, S, stellar	NPM1G -08.0602
NGC 7215	22 08 34.5	+00 30 44	Sa pec	14.9	13.9	1.1 × 0.4	vF, S, E	CGCG 377-31
NGC 7218	22 10 11.5	-16 39 38	SBc	12.7	12.0	2.6 × 1.1	pB, lE, r	MCG -3-56-8, IRAS 22074-1654
NGC 7220	22 11 30.9	-22 57 11	SB0	14.5	13.5	0.9 × 0.7	eF, vS, vlE, gbM, * 10 n 3'	ESO 532-28, MCG -4-52-20
NGC 7222	22 10 51.7	+02 06 23	SBb	14.6	13.8	1.2 × 1.2	vF, S	UGC 11934, MCG 0-56-12, CGCG 377-35, NPM1G +01.0542
NGC 7230	22 14 13.1	-17 04 28	SBbc	14.9	14.1	0.9 × 0.9	vF, S, R, bM	MCG -3-56-12, IRAS 22114-1719
NGC 7239	22 15 01.3	-05 03 10	E-S0	14.8	13.8	1.1 × 0.7	eF, vS	NPM1G -05.0643
NGC 7246	22 17 42.6	-15 34 12	Sa	15.4	14.5	1.5 × 0.8	vF, S, vlE, vgbM, * 13 n	IC 5198, MCG -3-56-14, IRAS 22150-1549
NGC 7247	22 17 41.1	-23 43 50	SBb	13.4	12.6	1.4 × 0.8	pF, vS, R, lbM, B D * p 13s	ESO 533-8, MCG -4-52-32, IRAS 22149-2358
NGC 7251	22 20 27.2	-15 46 23	Sa	13.5	12.6	1.9 × 1.7	F, pS, R, gpmbM	MCG -3-57-2, IRAS 22177-1601
NGC 7252	22 20 44.8	-24 40 42	SB0	12.1	11.4	2.1 × 1.7	F, S, R, er	ESO 533-15, MCG -4-52-36, Arp 226, IRAS 22179-2455, PRC D-35, AM 2217-245, Atoms for peace galaxy
NGC 7255	22 23 08.0	-15 32 28	S0-a	15.0	14.1	1.3 × 0.4	eF, L, mE 30°, sbMN	MCG -3-57-6, IRAS 22204-1547
NGC 7256	22 22 36.0	-21 44 05	SBb	14.0	13.2	1.3 × 0.6	3 F st in F neb	NGC 7254, ESO 602-13, KAZ 537, IRAS 22198-2159
NGC 7257	22 22 36.5	-04 07 15	SBbc	13.5	12.7	1.9 × 1.4	F, vS, lE	NGC 7260, MCG -1-57-3
NGC 7266	22 23 59.0	-04 04 23	Sa	14.3	13.4	0.9 × 0.7	F, vS, R, alm stellar	MCG -1-57-6, MK 910, IRAS 22213-0419
NGC 7269	22 25 46.8	-13 10 01	Sb	14.5	13.7	1 × 0.7	eF, pS, R, glbM	MCG -2-57-5, IRAS 22231-1325
NGC 7284	22 28 35.8	-24 50 40	SB0	13.1	12.1	2.3 × 1.6	cF, cS, lE, r, D * inv	ESO 533-31, MCG -4-53-4, VV 74, Arp 93, AM 2224-250
NGC 7285	22 28 37.8	-24 50 26	SBa	12.8	11.9	2.1 × 1.5	Neb * 1' dist from h 3943	ESO 533-32, MCG -4-53-5, VV 74, Arp 93, AM 2224-250
NGC 7287 A	22 28 48.9	-22 12 08	SB0	16.0	15.0	0.3 × 0.2	eF, slightly nebs D *	ESO 602-20A
NGC 7288	22 28 14.9	-02 53 05	S0-a	13.9	13.0	2.3 × 1.5	vF, eS, stellar	MCG -1-57-13, MK 912, IRAS 22256-0308
NGC 7298	22 30 50.6	-14 11 19	Sc	14.3	13.7	1.3 × 1.1	vF, pL, iR	MCG -2-57-10, MK 1124, IRAS 22281-1426
NGC 7300	22 30 59.9	-14 00 11	SBb	13.6	12.9	2.1 × 1	vF, cS, E, vglbM	MCG -2-57-11
NGC 7301	22 30 34.8	-17 34 25	SBab	14.2	13.4	1 × 0.5	vF, pS, lE, lbM	ESO 602-23, MCG -3-57-15, VV 372, IRAS 22278-1749
NGC 7302	22 32 23.9	-14 07 15	E-S0	13.2	12.3	1.8 × 1.1	F, pS, R, vsbMSN	IC 5228, MCG -2-57-13
NGC 7308	22 34 32.0	-12 56 01	E-S0	14.7	13.7	1.2 × 0.9	pB, vS, R	IC 1448, MCG -2-57-17
NGC 7309	22 34 20.6	-10 21 22	SBc	13.0	12.5	2 × 1.7	vF, pL, R, glbM, r	MCG -2-57-16, IRAS 22317-1036
NGC 7310	22 34 36.8	-22 29 06	SBbc	14.6	13.8	0.9 × 0.7	vF, pS, R, bMN	ESO 533-49, MCG -4-53-15, KAZ 544, IRAS 22318-2244
NGC 7341	22 39 05.6	-22 39 59	SBab	13.1	12.3	2.4 × 1	pF, pS, E, lbM	ESO 534-11, MCG -4-53-27
NGC 7344	22 39 36.1	-04 09 32	Sab	14.5	13.7	1.5 × 0.8	pF, vS, R	MCG -1-57-20
NGC 7349	22 41 14.7	-21 47 48	SBb	15.1	14.3	1 × 0.5	eF, vS, E 175°, biN, bn	ESO 603-4, MCG -4-53-29
NGC 7351	22 41 26.9	-04 26 39	S0	13.9	12.9	1.8 × 1	pF, pS, R, bM, r	MCG -1-57-22
NGC 7359	22 44 47.9	-23 41 17	S0	13.5	12.5	2.4 × 0.6	pF, vS, pmE, bMN	ESO 534-22, MCG -4-53-34
NGC 7364	22 44 24.2	-00 09 45	S0-a	13.5	12.6	1.8 × 1.1	F, S, R, psbM	UGC 12174, MCG 0-58-1, CGCG 379-2
NGC 7365	22 45 10.0	-19 57 06	E-S0	13.7	12.9	1.5 × 1	vF, eS, R, gbMN, * 11 nf 4'	ESO 603-10, MCG -3-58-1, NPM1G -20.0607
NGC 7371	22 46 03.6	-11 00 02	SB0-a	12.3	11.5	2 × 2	vF, pL, R, lbM	MCG -2-58-1, NPM1G -11.0516
NGC 7377	22 47 47.4	-22 18 41	SB0-a	12.1	11.1	3 × 2.5	pB, S, vlE, vgmbM, * 12 p	ESO 534-26, MCG -4-53-38, IRAS 22451-2234
NGC 7378	22 47 47.5	-11 49 00	SBab	13.5	12.7	1.5 × 0.9	vF, pL	MCG -2-58-5
NGC 7381	22 50 08.1	-19 43 29	Scd	14.9	14.2	0.7 × 0.5	eF, vS, R, gbM	ESO 603-17, MCG -3-58-7A
NGC 7391	22 50 36.0	-01 32 41	E1	13.1	11.9	1.7 × 1.5	cF, cS, R, sbM * 13, * np	UGC 12211, MCG 0-58-6, CGCG 379-8
NGC 7392	22 51 48.6	-20 36 31	SBbc	12.6	11.9	2.2 × 1.4	pB, pS, lE 120°, mbM	ESO 603-22, MCG -4-53-40
NGC 7393	22 51 38.2	-05 33 26	SBc/P	13.6	12.9	2 × 0.9	vF, pL, lE, vgbM, r	MCG -1-58-2, VV 68, Arp 15
NGC 7399	22 52 39.3	-09 16 03	S0-a	14.6	13.7	0.9 × 0.4	eF, pL	MCG -2-58-6
NGC 7406	22 53 56.4	-06 34 44	S?	14.5	13.6	1.1 × 0.6	F, S, lE	MCG -1-58-3
NGC 7416	22 55 41.6	-05 29 42	SBb	13.2	12.4	3.2 × 0.7	F, pL, pmE, vgbM	MCG -1-58-4
NGC 7425	22 57 15.6	-10 57 00	SB0-a	15.1	14.2	0.9 × 0.6	eF, vlE, * 10 p 4'	MCG -2-58-13
NGC 7441	22 56 41.4	-07 22 47	Sc	14.5	13.8	1.3 × 0.8	vF, pS, iR, * 10 p (? PD)	IC 1458, MCG -1-58-7
NGC 7443	23 00 08.7	-12 48 28	S0-a	12.6	11.6	1.4 × 0.5	F, vS, vlE, smbM, er, n of 2	MCG -2-58-15
NGC 7444	23 00 08.8	-12 50 03	S0	13.9	12.9	1.7 × 0.6	F, vS, vlE, smbM, er, s of 2	MCG -2-58-16
NGC 7450	23 00 47.7	-12 55 04	S0-a	14.0	13.1	1.8 × 1.8	vF, S	MCG -2-58-19, MK 1126
NGC 7491	23 08 06.0	-05 57 59	Sbc	14.6	13.8	1 × 0.7	vF, S, R, vlbM	MCG -1-59-2, IRAS 23054-0614
NGC 7494	23 08 58.4	-24 22 09	E1	15.6	14.6	0.8 × 0.7	eF, vS, stellar	ESO 535-5, MCG -4-54-7
NGC 7498	23 09 56.0	-24 25 28	Sab	15.2	14.4	0.9 × 0.4	vF, S, iR	ESO 535-6, MCG -4-54-8
NGC 7520	23 12 53.1	-23 28 08	Sa	14.1	13.2	1.3 × 0.8	F, pS, bet 2 st	IC 5290, ESO 535-8, MCG -4-54-14
NGC 7573	23 16 26.3	-22 09 14	SBc	14.5	13.7	1.3 × 1.1	eF, S, iR, b np, * 10 p 4'	ESO 604-8, MCG -4-54-17, NPM1G -22.0395, AM 2313-222
NGC 7576	23 17 22.7	-04 43 40	S0-a	13.7	12.9	1.3 × 0.9	F, S, smbM	MCG -1-59-12, IRAS 23148-0500
NGC 7585	23 18 01.3	-04 39 01	S0-a	12.3	11.4	2.3 × 2	pB, pS, iR, gbM	MCG -1-59-15, Arp 223
NGC 7592	23 18 22.0	-04 24 59	S0-a	14.4	13.5	1.1 × 0.9	eF, vS	MCG -1-59-17, MK 928, VV 731, IRAS 23157-0441
NGC 7596	23 17 12.0	-06 54 42	S0	15.2	14.2	1 × 0.5	vF, pS, lE 0°, lbMN	IC 1477, MCG -1-59-11, IRAS 23145-0711
NGC 7600	23 18 53.8	-07 34 48	E-S0	12.9	12.0	2.5 × 1	cF, S, R, psmbM	MCG -1-59-19
NGC 7606	23 19 04.8	-08 29 11	Sb	11.5	10.8	5.4 × 2.1	pF, cL, pmE 0° ±	MCG -2-59-12, IRAS 23164-0845
NGC 7646	23 24 06.9	-11 51 37	Sc	14.0	13.3	0.9 × 0.6	vF, vS, E 260° (neb?), * 9 n 3'.6	IC 5318, MCG -2-59-15, IRAS 23215-1208
NGC 7656	23 24 31.5	-19 03 33	S0	14.5	13.5	1.2 × 1.1	vF, vS, R, bMN	ESO 605-5, MCG -3-59-8, VV 669, NPM1G -19.0676
NGC 7665	23 27 14.8	-09 23 11	Sm	13.9	13.3	0.7 × 0.7	eF, S, stellar	MCG -2-59-19, IRAS 23246-0939
NGC 7692	23 32 46.7	-05 35 46	Irr	15.4	14.8	0.5 × 0.4	Neb, * 9 f 18s, 73" s	MCG -1-60-3, IRAS 23302-0552
NGC 7709	23 35 27.2	-16 42 20	SB0	13.6	12.6	2.3 × 0.6	pF, S, R, lbM	MCG -3-60-2, IRAS 23328-1658
NGC 7717	23 37 43.6	-15 07 07	SB0-a	13.7	12.8	1.4 × 1.2	vF, S	MCG -3-60-8
NGC 7719 1	23 38 02.6	-22 58 29	Sab	15.0	14.2	0.9 × 0.7	eF, vS, R	ESO 536-12, IRAS 23354-2315
NGC 7719 2	23 38 02.5	-22 58 40	S	17.0	16.2	0.2 × 0.1	eF, vS, R
NGC 7721	23 38 48.6	-06 31 04	Sc	12.2	11.6	2.8 × 1.1	pF, cL, E 12° ±, vgbM	MCG -1-60-17, IRAS 23362-0647
NGC 7723	23 38 57.0	-12 57 40	SBb	11.9	11.2	3.5 × 2.2	cB, cL, E, gmbM, r	MCG -2-60-5, IRAS 23363-1314
NGC 7724	23 39 07.0	-12 13 27	Sb	13.7	12.9	1.5 × 1	eF, pL, iR	MCG -2-60-6
NGC 7725	23 39 14.7	-04 32 20	S0	14.8	13.8	0.8 × 0.7	eeF	MCG -1-60-18, IRAS 23367-0448
NGC 7727	23 39 53.7	-12 17 34	SBa/P	11.5	10.6	4.7 × 3.5	pB, pL, iR, mbM	MCG -2-60-8, VV 67, Arp 222, IRAS 23367+2651
NGC 7730	23 40 45.8	-20 30 32	Sc	14.9	14.0	0.7 × 0.6	pB, pL, E	ESO 606-2, MCG -4-55-22, IRAS 23381-2047
NGC 7736	23 42 25.7	-19 27 09	S0	13.9	12.9	1.7 × 1.5	eF, eS, gbM, bet 2 st 12	ESO 606-5, MCG -3-60-10, NPM1G -19.0695
NGC 7754	23 49 11.2	-16 36 02	Sa	15.4	14.5	0.6 × 0.3	eF, vS	MCG -3-60-21, IRAS 23466-1652
NGC 7754 A	23 49 06.4	-16 34 45	S0	16.5	15.5	0.4 × 0.2	eF, vS
NGC 7758	23 48 55.1	-22 01 27	E/SB0	15.1	14.1	0.7 × 0.5	eF, vS, iR, sbM, D * 10 nf 50s	ESO 606-10, NPM1G -22.0413
NGC 7759	23 48 54.6	-16 32 27	SB0	14.0	13.0	1.3 × 0.9	vF, S, R, lbM, B * n	MCG -3-60-18
NGC 7759 A	23 48 56.8	-16 32 26	S	15.6	14.8	0.6 × 0.2	vF, S, R, lbM, B * n	MCG -3-60-19
NGC 7761	23 51 28.8	-13 22 52	S0	14.1	13.1	1.2 × 1.2	F, vS, R, gbM, * 10 p 8'	IC 5361, MCG -2-60-20, NPM1G -13.0659, IRAS 23488-1339
NGC 7763	23 50 15.7	-16 35 23	E-S0	15.3	14.3	0.7 × 0.4	eF, vS, R, F * f	NPM1G -16.0627
NGC 7776	23 54 16.5	-13 35 11	Sa	14.8	13.9	0.9 × 0.3	eF, vS, lE, gbM	IC 1514, MCG -2-60-22
IC 1330	20 46 14.8	-14 01 22	Sc	14.7	14.0	1.2 × 0.4	F, vS, dif	MCG -2-53-2, IRAS 20434-1412
IC 1331	20 47 48.8	-09 59 44	S0-a	14.6	13.7	1.8 × 0.6	F, S, bM, r	MCG -2-53-5
IC 1332	20 51 51.3	-13 42 40	Sb	14.3	13.5	0.9 × 0.6	F, vS, R	MCG -2-53-11, NPM1G -13.0503
IC 1341	21 00 16.6	-13 58 33	S0	15.3	14.3	0.5 × 0.3	F, vS, R, lbM	MCG -2-53-16, NPM1G -14.0591
IC 1342	21 00 25.5	-14 29 42	Sc	14.6	13.9	0.8 × 0.3	vF, vS, E pf, lbM	MCG -3-53-17, IRAS 20576-1441
IC 1344	21 01 16.5	-13 22 49	S	14.5	13.7	1 × 0.4	pB, pL, iF, sbM	MCG -2-53-18
IC 1345	21 01 22.1	-13 23 51	E0	15.6	14.6	0.5 × 0.5	vF, S, R, vlbM	NPM1G -13.0508
IC 1346	21 01 37.1	-13 57 37	SBb	14.9	14.1	1.2 × 0.6	pB, vS, R, gbM	MCG -2-53-19
IC 1347	21 01 44.3	-13 18 46	S0	15.3	14.4	0.8 × 0.6	pB, R	MCG -2-53-20, NPM1G -13.0510
IC 1348	21 01 43.9	-13 21 25	S0	15.3	14.3	0.8 × 0.4	F, vS, R, bM	NPM1G -13.0509
IC 1349	21 01 50.4	-13 15 54	S	15.5	14.7	0.6 × 0.3	vF, vS, R, lbM	NPM1G -13.0511
IC 1351	21 01 52.3	-13 12 05	S0	15.7	14.7	0.5 × 0.2	F, vS, R, lbM	NPM1G -13.0512
IC 1352	21 01 54.8	-13 23 04	S	16.5	15.7	0.3 × 0.1	pB
IC 1353	21 01 56.3	-13 16 21	S	16.5	15.7	0.3 × 0.2	vF, vS, R
IC 1354	21 01 52.2	-13 51 08	S	16.0	15.2	0.7 × 0.4	F, vS, R, bM	IC 1350, MCG -2-53-21, NPM1G -14.0595
IC 1355	21 01 58.3	-13 10 21	E0	15.3	14.3	0.4 × 0.4	F, vS, R, bM	NPM1G -13.0513
IC 1357	21 05 57.2	-10 42 57	Sa	15.2	14.3	1.3 × 0.7	vF, vS, iF, vlbM	NPM1G -10.0600
IC 1362	21 11 52.6	+02 19 46	E?	15.6	14.6	0.3 × 0.2	vF, vS, R, * 14 nf	CGCG 375-7, KARA 898, NPM1G +02.0485
IC 1366	21 14 07.9	+01 46 36	S	15.3	14.5	0.4 × 0.2	F, S, iR, bet 2 st 11 & 13	CGCG 375-17, NPM1G +01.0513
IC 1368	21 14 12.6	+02 10 42	Sa	14.3	13.4	1.2 × 0.4	eeF, S, R, v diffic	UGC 11703, MCG 0-54-8, CGCG 375-18, IRAS 21116+0158
IC 1370	21 15 14.3	+02 11 32	5C	15.1	14.6	1.6 × 0.5	vF, 2 F st inv	CGCG 375-21, 2ZW 111
IC 1371	21 20 15.6	-04 52 34	E-S0	14.8	13.8	0.9 × 0.7	F, S, dif, gbM, r	MCG -1-54-13, NPM1G -05.0598
IC 1372	21 20 17.1	-05 36 17	S	15.5	14.7	0.8 × 0.4	vF, vS, R, dif, * 14 sf
IC 1373	21 20 37.1	+01 05 35	S0	15.5	14.5	0.3 × 0.3	F, vS, R, sbM, 2 others south	MCG 0-54-13, CGCG 375-29, NPM1G +00.0565
IC 1374	21 21 02.6	+01 42 49	S?	15.9	15.1	0.3 × 0.2	vF, vS, lbM	CGCG 375-31, KARA 908, NPM1G +01.0518
IC 1381	21 27 33.6	-01 11 17	SB	15.4	14.6	0.8 × 0.5	F, vS, R, bM	MCG 0-54-16, CGCG 375-36, NPM1G -01.0541
IC 1383	21 27 39.5	-01 06 08	S	15.3	14.5	0.4 × 0.2	F, vS, R, stellar	CGCG 375-37
IC 1384	21 27 53.0	-01 22 07	Irr	15.4	14.7	0.7 × 0.5	vF, vS, R	MCG 0-54-17, CGCG 375-39
IC 1385	21 28 51.1	-01 04 11	SB?	15.8	15.0	0.4 × 0.4	pB, vS, R	MCG 0-54-22, CGCG 375-42
IC 1387	21 29 34.4	-01 21 02	E3	15.5	14.5	0.4 × 0.3	pB, vS, iF	MCG 0-54-26, CGCG 375-45, ARAK 547, NPM1G -01.0544
IC 1388	21 29 52.1	-00 37 51	S	15.0	14.2	0.4 × 0.2	eF, vS, 2 st nf	MCG 0-54-27, CGCG 375-46, ARAK 548, NPM1G -00.0561
IC 1390	21 32 24.9	-01 51 43	SBc	15.5	14.5	0.7 × 0.6	F, vS, R, bM	MCG 0-55-4, CGCG 376-5
IC 1391	21 35 00.4	-00 30 41	E?	15.7	14.7	0.2 × 0.2	vF, S, dif	MCG 0-55-7, CGCG 376-10
IC 1397	21 44 02.2	-04 53 04	S	15.3	14.5	0.7 × 0.3	F, vS, stellar	NPM1G -05.0614
IC 1401	21 46 59.5	+01 42 41	Sbc	14.4	13.8	1.8 × 0.7	pB, pS, r	UGC 11810, MCG 0-55-15, CGCG 376-31, KARA 930, IRAS 21444+0128
IC 1403	21 50 29.0	-02 42 56	S	16.6	15.8	0.5 × 0.3	eF, S, F, * att, v diffic	NPM1G -02.0472
IC 1405	21 50 49.8	+02 01 17	SBab	14.6	13.8	0.9 × 0.7	pB, vS, R, bM	UGC 11826, MCG 0-55-20, CGCG 376-37, NPM1G +01.0534
IC 1406	21 51 04.8	+01 59 15	E0	15.7	14.7	0.3 × 0.3	F, vS, R, stellar	CGCG 376-38, NPM1G +01.0535
IC 1409	21 53 19.5	-07 29 59	S	16.0	15.2	0.5 × 0.3	eF, S, iF
IC 1410	21 56 02.1	-02 53 59	E4	15.9	14.9	0.5 × 0.3	pF, vSN	NPM1G -03.0616
IC 1411	21 56 00.5	-01 31 00	E4	14.4	13.4	0.9 × 0.5	F, vS, R, vlbM	UGC 11850, MCG 0-56-1, CGCG 377-1, NPM1G -01.0553
IC 1413 1	21 58 25.3	-03 07 29	S/P	16.5	15.7	0.9 × 0.2	F, S, stellar
IC 1413 2	21 58 26.8	-03 06 06	S	16.0	15.2	0.7 × 0.2	F, S, stellar
IC 1417	22 00 21.7	-13 08 49	Sb	14.5	13.7	1.3 × 0.4	pB, pL, part more condensed	MCG -2-56-3, IRAS 21576-1323
IC 1419	22 02 58.8	-09 55 14	S	16.0	15.2	0.4 × 0.2	eF, slbM	NPM1G -10.0646
IC 1421	22 03 03.9	-09 58 40	E3	15.8	14.8	0.4 × 0.3	Neb * 14m	MCG -2-56-9, NPM1G -10.0647
IC 1430	22 07 29.7	-13 34 51	E0	16.0	15.0	0.4 × 0.4	F, S, vlbM, diffic
IC 1431	22 07 39.5	-13 30 48	Sa	15.1	14.2	0.8 × 0.7	eF, v diffic, F * np	MCG -2-56-15
IC 1433	22 12 10.5	-12 45 54	P	15.7	14.7	0.7 × 0.5	F, S, E pf, bM	MCG -2-56-21, VV 390, NPM1G -13.0565
IC 1435	22 13 26.1	-22 05 47	Sbc	13.9	13.1	1 × 0.6	F, S	ESO 601-30, MCG -4-52-25, AM 2210-222, IRAS 22106-2220
IC 1436	22 13 51.3	-10 11 29	E-S0	15.8	14.8	0.7 × 0.6	eF, vS, R, vSN	MCG -2-56-24, NPM1G -10.0652
IC 1437	22 15 44.9	+02 03 57	S0-a	14.4	13.5	1.1 × 1	pB, vS, R, mbM	UGC 11965, MCG 0-56-16, CGCG 377-42, KARA 956
IC 1438	22 16 29.0	-21 25 51	SBa	12.8	11.9	2.4 × 2.1	F, biN	ESO 602-1, MCG -4-52-29, IRAS 22137-2140
IC 1439	22 16 40.2	-21 29 08	SBa	14.6	13.7	1.3 × 0.9	vF, S, vlbM	ESO 602-2, MCG -4-52-30
IC 1440	22 16 33.2	-16 00 59	E?	14.9	13.9	1.2 × 0.3	F, S, stellar	MCG -3-56-13
IC 1443	22 19 03.6	-20 56 24	E2	13.5	12.5	0.8 × 0.7	pB, S, iF, mbM	ESO 602-5, MCG -4-52-33
IC 1445	22 25 30.2	-17 14 37	E-S0	13.5	12.7	1.6 × 1.3	pF, vS, gbMN	ESO 602-19, MCG -3-57-7
IC 1446	22 29 04.6	-01 11 03	S	15.9	15.1	0.6 × 0.3	vF, stellar	NPM1G -01.0563
IC 1447	22 29 59.8	-05 07 10	Sb	13.6	12.8	1.5 × 0.8	eeF, pS, R, * 9.0 n 3'	MCG -1-57-14, IRAS 22273-0522
IC 1449	22 35 07.0	-08 45 56	S	15.8	15.0	0.5 × 0.4	F, S, iF, bM, r
IC 1451	22 46 07.4	-10 22 13	Sc	14.9	14.2	0.5 × 0.5	vF, S, dif, vS, excent N	MCG -2-58-2
IC 1453	22 46 54.4	-13 26 58	SBb	15.1	14.3	0.7 × 0.6	pB, pL, R	MCG -2-58-4
IC 1456	22 55 18.2	-12 43 55	S0	16.0	15.0	0.7 × 0.2	vF, vS
IC 1464 A	23 03 11.0	-08 59 19	S M	15.4	14.6	0.7 × 0.4	F, r, D ?	MCG -2-58-20, NPM1G -09.0723
IC 1464 B	23 03 12.0	-08 59 32	S M	15.7	14.9	0.5 × 0.3	F, r, D ?	MCG -2-58-21, NPM1G -09.0724
IC 1469	23 06 28.5	-13 32 11	E4	16.0	15.0	0.5 × 0.3	F, S, R, F * f
IC 1471	23 08 45.0	-12 38 21	S?	14.5	13.6	0.8 × 0.4	pB, S, R, bM	MCG -2-59-3
IC 1479	23 18 46.3	-10 23 55	E-S0	14.7	13.7	1.1 × 1	pF, S, R, stellar	MCG -2-59-10, NPM1G -10.0713
IC 1489	23 26 32.1	-12 30 59	S	15.0	14.2	0.4 × 0.2	F, vS, R, * 9 south	MCG -2-59-16, IRAS 23239-1247
IC 1491	23 29 24.5	-16 18 58	S?	15.0	14.1	0.5 × 0.3	F, S, R	MCG -3-59-10
IC 1494	23 30 46.1	-12 43 27	S	15.9	15.1	0.5 × 0.2	F, R, lbM	NPM1G -13.0644
IC 1498	23 31 53.5	-05 00 23	Sa	14.6	13.7	1.9 × 0.6	eeF, pS, R, * 9.5 p 36s, 3' s	MCG -1-60-2
IC 1505	23 41 37.0	-03 33 53	E2	14.7	13.7	0.9 × 0.7	eeF, pS, R, 3 st f, diffic	MCG -1-60-20, NPM1G -03.0698
IC 1509	23 47 16.6	-15 18 26	Sc	15.2	14.5	1.4 × 0.2	F, S, E ns, gbM	MCG -3-60-14
IC 5050	20 45 15.0	-05 37 23	Sb	14.3	13.5	1.3 × 0.9	F, cS, dif, vS E N	MCG -1-53-5, IRAS 20426-0548
IC 5089	21 10 54.4	-03 51 44	S	16.0	15.2	0.7 × 0.3	eF, vS, bM, F * 30" sp	NPM1G -04.0559
IC 5090	21 11 30.6	-02 01 55	Sa	14.4	13.5	1.2 × 0.5	vF, S, R, sbM	UGC 11691, MCG 0-54-3, CGCG 375-6, IRAS 21089-0214
IC 5111	21 28 10.9	+02 28 28	S?	15.3	14.4	0.7 × 0.6	F, S, iF	MCG 0-54-21, CGCG 375-41, KARA 917
IC 5126	21 40 28.6	-06 20 45	Sb	15.7	14.9	0.5 × 0.5	vF, vS, R, bet 2 st 14
IC 5178	22 12 33.2	-22 57 16	SB+C?	14.7	13.8	1.1 × 0.8	eF, vS, 7220 p 63s	ESO 532-31, MCG -4-52-22
IC 5210	22 22 31.1	-18 52 09	E-S0	14.0	13.0	1.2 × 1.1	eeF, vS, R, p of 2	ESO 602-12, MCG -3-57-4
IC 5211	22 22 42.9	-18 52 47	Sab	14.3	13.5	1 × 0.6	eF, S, f of 2	ESO 602-14, MCG -3-57-5
IC 5241	22 41 38.5	+02 38 23	SBc	14.6	13.9	1 × 0.8	pB, cS, R, gbM, r	UGC 12152, MCG 0-57-8, CGCG 378-16, KUG 2239+023
IC 5261	22 54 25.2	-20 21 48	SBc	13.9	13.2	1.5 × 1.3	eeF, pL, R, v diffic, * 9 p 22s	ESO 603-26, MCG -4-54-1, IRAS 22517-2037
IC 5278	23 00 15.9	-08 10 43	Sd	15.8	15.2	1.2 × 0.4	eF (not verified)	MCG -1-58-14
IC 5304	23 18 52.5	-10 15 32	E-S0	14.4	13.4	1.4 × 0.9	eF, S, R, 3 or 4 F st sp	MCG -2-59-11, NPM1G -10.0714
IC 5310	23 20 47.7	-22 08 56	E0	15.8	14.8	0.5 × 0.5	eF, eS, alm stell, * 9.5 n 5'	ESO 605-1, NPM1G -22.0398
IC 5321	23 26 20.0	-17 57 24	Sa	13.9	13.0	1.3 × 0.8	eF, vS, R, * 10 np 1'	ESO 605-7, MCG -3-59-9, IRAS 23237-1813
IC 5327	23 30 47.5	-13 29 07	Sb	14.1	13.3	1.4 × 1	pF, pS, * 11 f 1'	IC 1495, MCG -2-59-24, IRAS 23281-1345
IC 5334	23 34 36.4	-04 32 02	Sab	14.1	13.3	1.8 × 0.6	Neb * 10.5 (? close D *)	MCG -1-60-8
IC 5343	23 39 22.4	-22 29 50	Irr	14.0	13.6	0.8 × 0.6	eF, pS, * 7.5 sf 19s	ESO 536-15, MCG -4-55-19
IC 5345	23 39 32.3	-22 24 48	Sbc	14.5	13.7	0.8 × 0.6	vF, 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]
PNG	RA	Dec	Main ID	PK	IRAS	Discoverer	Identities	oDiam ["]	rDiam ["]	Dist [kpc]	Rvel [km/s]	ExpVel [km/s]	C* Name	C* Mag	C* SP Type
PN G036.1-57.1	22 29 39	-20 50 15	NGC 7293	36-57.1	22267-2102	CURTIS 1918	ARO 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. 1	U: 11.81, B: 13.10, V: 13.50	Hg O(H)
PN G037.7-34.5	21 04 11	-11 21 57	NGC 7009	37-34.1	21014-1133	HERSCHEL 1782	ARO 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 27614	B: 12.66, V: 12.78	O(H)

«A Catalog of Parameters for Globular Clusters in the Milky Way» William E. Harris, 1996 ^[148]
ID	Name	RA	Dec	R_Sun [kpc]	R_GC [kpc]	Fe/H	wt	E_B-V	V_HB	(m-M)V	V_t	M_V,t	U-B	B-V	V-R	V-I	spt	ellip	v_r [km/s]	v_LSR [km/s]	sig_v [km/s]	c	r_c [']	r_h [']	μ_V	ρ₀	lg(tc)	lg(th)
NGC 6981	M 72	20 53 27.70	-12 32 14.3	17.0	12.9	-1.42	4	0.05	16.90	16.31	9.27	-7.04	0.14	0.72	0.45	0.94	F7	0.02	-345.0 ± 3.7	-336.2		1.21	0.46	0.93	19.02	2.38	8.72	9.23
NGC 7089	M 2	21 33 27.02	-00 49 23.7	11.5	10.4	-1.65	5	0.06	16.05	15.50	6.47	-9.03	0.09	0.66	0.46	0.92	F4	0.11	-5.3 ± 2.0	3.8	8.2 ± 0.6	1.59	0.32	1.06	15.78	4.00	8.48	9.40
NGC 7492		23 08 26.63	-15 36 41.4	26.3	25.3	-1.78	5	0.00	17.63	17.10	11.29	-5.81	0.23	0.42				0.24	-177.5 ± 0.6	-176.2	1.2 ± 1.0	0.72	0.86	1.15	20.68	1.27	9.60	9.44

7	«Der grosse Kosmos-Himmelsführer» von Ian Ridpath und Wil Tirion; Kosmos Verlag; ISBN 3-440-05787-9
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10	«dtv-Atlas zur Astronomie» von Joachim Herrmann; Deutscher Taschenbuch Verlag; ISBN 3-423-03006-2
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20	«Sternbilder und ihre Mythen» von Gerhard Fasching; Zweite, verbesserte Auflage; Springer Verlag Wien, New York; ISBN 3-211-82552-5 (Wien); ISBN 0-387-82552-5 (New York)
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150	IAU: The Constellations, 11. Oktober 2020; iau.org/public/themes/constellations
154	Yale Bright Star Catalog, 15. Oktober 2020; tdc-www.harvard.edu/catalogs/bsc5.html
277	«Historische Deep-Sky Kataloge» von Dr. Wolfgang Steinicke; klima-luft.de/steinicke (2021-02-17)