The open cluster Messier 6 in the constellation Scorpius is also known as the Butterfly Cluster or NGC 6405
This is a list of open clusters located in the Milky Way . An open cluster is an association of up to a few thousand stars that all formed from the same giant molecular cloud . There are over 1,000 known open clusters in the Milky Way galaxy, but the actual total may be up to ten times higher.[ 1] The estimated half-lives of clusters, after which half the original cluster members will have been lost, range from 150 million to 800 million years, depending on the original density.[ 2]
Cluster identifier
Constellation
Distance (parsecs )
Age (Myr )
Diameter
Apparent magnitude
Notes
Epoch J2000
R. A.
Dec.
Hyades
04h 26.9m
+15° 52′
Taurus
47
625
330'
0.5
[ 3]
Coma Star Cluster
12h 22.5m
+25° 51′
Coma Berenices
86
400-500
120'
1.8
[ 4]
Trapezium Cluster
5h 35.4m
−05° 27′
Orion
412
0.3
0.783'
4.0
[ 5]
Messier 6, Butterfly Cluster
17h 40.1m
−32° 13′
Scorpius
487
94
20'
4.2
[ 1]
Messier 7
17h 53.8m
−34° 47′
Scorpius
280
224
80'
3.3
[ 6] [ 7]
Messier 11, Wild Duck Cluster
18h 51.1m
−06° 16′
Scutum
1,900
250
13'
5.8
[ 1] [ 7] [ 8]
Messier 16, Eagle Nebula
18h 18.8m
−13° 49′
Serpens
1,800
1.3
6'
6.0
[ 1]
Messier 18
18h 20.0m
−17° 06′
Sagittarius
1,296
17
5'
6.9
[ 1]
Messier 21
18h 04.2m
−22° 29′
Sagittarius
1,205
12
14'
5.9
[ 1]
Messier 23
17h 57.0m
−18° 59′
Sagittarius
628
300
30'
5.5
[ 1] [ 7]
Messier 24
18h 17.0m
−18° 29′
Sagittarius
3,070
220
90'
2.5
[ 1] [ 7]
Messier 25
18h 31.7m
−19° 07′
Sagittarius
620
92
30'
4.6
[ 1]
Messier 26
18h 45.3m
−09° 23′
Scutum
1,600
85
7'
8.0
[ 1]
Messier 34
02h 42.1m
+42° 46′
Perseus
499
180
36'
5.2
[ 1] [ 7]
Messier 35
06h 09.1m
+24° 21′
Gemini
912
180
25'
5.0
[ 9]
Messier 36
05h 36.2m
+34° 08′
Auriga
1,330
25
10'
6.0
[ 1]
Messier 37
05h 52.3m
+32° 33′
Auriga
1,400
347
14'
5.6
[ 1]
Messier 38
05h 28.7m
+35° 51′
Auriga
1,400
316
20'
6.4
[ 1]
Messier 39
21h 31.8m
+48° 27′
Cygnus
311
280
30'
4.6
[ 1] [ 6]
Messier 41
06h 46.0m
−20° 46′
Canis Major
710
240
40'
4.5
[ 1] [ 7]
Messier 44, Beehive Cluster
08h 40.4m
+19° 41′
Cancer
187
830
70'
3.1
[ 10] [ 11]
Messier 45, Pleiades
03h 47.4m
+24° 07′
Taurus
136
125
120'
1.2
[ 12]
Messier 46
07h 41.7m
−14° 49′
Puppis
1,510
250
20'
6.1
[ 1]
Messier 47
07h 36.6m
−14° 30′
Puppis
490
73
25'
4.4
[ 1]
Messier 48
08h 13.7m
−05° 45′
Hydra
770
400
30'
5.8
[ 1]
Messier 50
07h 02.6m
−08° 23′
Monoceros
1,000
130
14'
5.9
[ 9]
Messier 52
23h 24.8m
+61° 35′
Cassiopeia
1,400
160
15
6.9
[ 1]
Messier 67
08h 51.3m
+11° 48′
Cancer
908
4,000
25'
6.9
[ 1] [ 7]
Messier 93
07h 44.6m
−23° 52′
Puppis
1037
390
10'
6.2
[ 1]
Messier 103
01h 33.4m
+60° 39′
Cassiopeia
3,000
16
5'
7.4
[ 13]
IC 2602 , Southern Pleiades
10h 43.2m
−64° 24′
Carina
167
30
100'
1.9
[ 14]
IC 2391 , Omicron Velorum Cluster
08h 40.6m
−53° 02′
Vela
176
30
60'
2.5
[ 14]
NGC 2451 A
07h 45.4m
−37° 58′
Puppis
189
50
45'
2.8
[ 6] [ 15]
Alpha Persei Cluster
03h 26.0m
+49° 07′
Perseus
172
50
300'
1.2
[ 16]
Arp-Madore 2
07h 38.8m
−33° 51′
Puppis
8,870
5,000
1.3'
[ 17]
Blanco 1
00h 04.3m
−29° 56′
Sculptor
253
100
90'
4.5
[ 14]
Hodge 301
05h 38.5m
−69° 04′
Dorado
51,400
25
0.5'
11
[ 18] [ 19]
Lambda Orionis Cluster
05h 35m
+09° 56′
Orion
438
5
2.8
[ 20]
Pi Puppis Cluster
07h 08m
−37° 10′
Puppis
319
50'
2.1
[ 21]
Melotte 186
18h 01.1m
+02° 54′
Ophiuchus
200
100
240'
3.0
[ 22]
NGC 2070
05h 38.7m
−69° 06′
Dorado
48,500
1.5
3.5'
7.25
[ 23] [ 24]
NGC 2232
06h 26.4m
−04° 45′
Monoceros
325
53
45'
3.9
[ 1] [ 6]
IC 4756
18h 39.0m
−05° 27′
Serpens
330
500
40'
4.6
[ 1] [ 6]
NGC 2516 , Southern Beehive Cluster
07h 58.0m
−60° 48′
Carina
346
141
30'
3.8
[ 6] [ 7]
IC 4665
17h 46.3m
+05° 43′
Ophiuchus
352
43
70'
4.2
[ 1]
Trumpler 10
08h 47.8m
−42° 29′
Vela
365
35
14'
4.6
[ 1] [ 6]
NGC 6633
18h 27.7m
+06° 34′
Ophiuchus
375
660
20'
4.6
[ 25]
IC 348
03h 44.6m
+32° 10′
Perseus
385
44
7'
7.3
[ 1]
NGC 752
01h 57.7m
+37° 47′
Andromeda
400
1,700–2,000
75'
5.7
[ 26]
NGC 3532 , Wishing Well Cluster
11h 06.4m
−58° 40′
Carina
405
316
50'
3.0
[ 6] [ 7]
Collinder 121
07h 08m
−37° 10′
Canis Major
600
50'
2.6
[ 27]
Collinder 140
07h 24.5m
−31° 51′
Canis Major
410
35
42'
3.5
[ 1] [ 6]
Collinder 261
12h 38.0m
−68° 22′
Musca
2,500
8,000
9'
10.7
[ 28] [ 29]
NGC 2547
08h 10.8m
−49° 18′
Vela
433
38
25'
4.7
[ 6]
NGC 6281
17h 04.7m
−37° 59′
Scorpius
479
220
8'
5.4
[ 1]
NGC 225
00h 43.6m
+61° 46′
Cassiopeia
657
130
12'
7.0
[ 1]
NGC 5662
14h 35.6m
−56° 37′
Centaurus
666
70
30'
5.5
[ 1] [ 7]
NGC 5460
14h 07.4m
−48° 20′
Centaurus
678
160
36'
5.6
[ 1] [ 7]
NGC 189
00h 39.7m
+61° 04′
Cassiopeia
752
10
3.7'
8.8
[ 1]
NGC 6025
16h 03.3m
−60° 26′
Triangulum Australe
756
130
14'
5.1
[ 1] [ 7]
IC 5146
21h 53.5m
+47° 16′
Cygnus
852
1
9'
7.2
[ 1]
NGC 2301
06h 51.75m
+00° 28′
Monoceros
858
165
12'
6.0
[ 30]
IC 4651
17h 24.8m
−49° 56′
Ara
888
1,900
10'
6.9
[ 1] [ 7]
NGC 6087 , S Normae Cluster
16h 18.8m
−57° 56′
Norma
891
70
14'
5.4
[ 1] [ 7]
NGC 3114
10h 02.7m
−60° 07′
Carina
911
124
36'
4.2
[ 1]
NGC 2509
08h 00.7m
−19° 04′
Puppis
912
Uncertain[ 31]
10'
9.3
[ 32]
NGC 2264
06h 41.0m
+09° 53′
Monoceros
913
1.5
40'
3.9
[ 33]
NGC 1502
04h 07.8m
+62° 20′
Camelopardalis
1,000
10
8'
5.7
[ 1]
Berkeley 59
00h 04.0m
+68° 35′
Cepheus
1,000
2
180'
[ 34]
NGC 2169
06h 08.4m
+13° 58′
Orion
1,052
12
5'
5.9
[ 1]
NGC 6242
16h 55.6m
−39° 28′
Scorpius
1,131
50
9'
6.4
[ 1] [ 7]
NGC 381
01h 08.3m
+61° 35′
Cassiopeia
1,148
320
7'
9.3
[ 1]
NGC 6204
16h 46.1m
−47° 01′
Ara
1,200
79
6'
8.2
[ 1]
NGC 6231
16h 54.1m
−41° 50′
Scorpius
1,243
6
14'
2.6
[ 1] [ 7]
NGC 2439
07h 40.8m
−31° 41′
Puppis
1,300
25
9'
6.9
[ 1] [ 7]
NGC 6067
16h 13.2m
−54° 13′
Norma
1,417
170
14'
5.6
[ 1] [ 7]
NGC 2362 , Tau Canis Majoris Cluster
07h 18.6m
−24° 59′
Canis Major
1,480
4–5
5'
4.1
[ 35]
NGC 6756
19h 08.7m
+04° 42′
Aquila
1,507
62
4'
4.5
[ 1]
NGC 6031
16h 07.9m
−54° 03′
Norma
1,510
117
3'
8.5
[ 1] [ 36]
NGC 2175
06h 09.7m
+20° 29′
Orion
1,627
8.9
5'
6.8
[ 1]
NGC 188
00h 48.4m
+85° 15′
Cepheus
1,660
6,600
17'
8.1
[ 7] [ 37]
NGC 2244
06h 31.9m
+04° 56′
Monoceros
1,660
1.9
30'
4.8
[ 1]
NGC 129
00h 30.0m
+60° 13′
Cassiopeia
1,670
76
21′
6.5
[ 38]
NGC 2360 , Caroline's Cluster
07h 17.7m
−15° 38′
Canis Major
1,887
1,000
13'
7.2
[ 1] [ 7]
NGC 6834
19h 52.2m
+29° 25′
Cygnus
1,930
76
5'
7.8
[ 1] [ 36]
NGC 659
01h 44.4m
+60° 40′
Cassiopeia
1,938
35
5'
7.9
[ 1]
NGC 4755, Jewel Box
12h 53.6m
−60° 22′
Crux
1,976
14
10'
4.2
[ 1] [ 7]
NGC 6200
16h 44.1m
−47° 28′
Ara
2,056
8.5
12'
7.4
[ 39]
NGC 869
02h 19.1m
+57° 09′
Perseus
2,079
12
18'
3.7
[ 1]
NGC 637
01h 43.0m
+64° 02′
Cassiopeia
2,160
10
4.2'
8.2
[ 1]
NGC 2355
07h 17.0m
+13° 47′
Gemini
2,200
955
5'
9.7
[ 1] [ 7]
NGC 2129
06h 01.1m
+23° 19′
Gemini
2,200
10
5'
6.7
[ 1] [ 40]
NGC 663
01h 46.1m
+61° 14′
Cassiopeia
2,420
25
14'
7.1
[ 1]
NGC 457
01h 19.1m
+58° 17′
Cassiopeia
2,429
21
20'
6.4
[ 41]
NGC 2204
06h 15.5m
−18° 40′
Canis Major
2,629
787
13'
8.6
[ 1]
NGC 884
02h 22.0m
+57° 08′
Perseus
2,940
14
18'
3.8
[ 1] [ 7]
NGC 1931
05h 31.0m
+34° 15′
Auriga
3,086
10
3'
10.1
[ 1]
NGC 1980
5h 25.43m
−05° 54′
Orion
550
4.7
14'
2.5
[ 42]
NGC 2158
06h 07.4m
+24° 06′
Gemini
5,071
1,054
5'
8.6
[ 1]
Teutsch 2
05h 41.4m
+39° 14′
Auriga
5,700
900
2'
11
[ 43]
NGC 6791
19h 20.9m
+37° 46′
Lyra
5,853
8,900
16'
9.5
[ 1] [ 7]
NGC 3293
10h 35.8m
−58° 13′
Carina
2,750
8
8'
4.7
NGC 3766 , Pearl Cluster
11h 36.2m
−61° 37′
Centaurus
1745
14
12'
5.3
NGC 7419
22h 54.3m
+60° 48.9′
Cepheus
2,800
2'
13
NGC 7789 , White Rose Cluster
23h 57.4m
+56° 43′
Cassiopeia
2,337
1,700
16'
6.7
[ 44]
Gaia 1
06h 45.9m
−16° 45′
Canis Major
4,600
6,300
13'
8.3
Ru 7
06h 58.9m
−13° 15′
Canis Major
[citation needed ]
See also
References
^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk bl Dias W.S.; Alessi B.S.; Moitinho A.; Lepine J.R.D. (July 2002). "New catalog of optically visible open clusters and candidates". Astronomy and Astrophysics . 389 (3): 871– 873. arXiv :astro-ph/0203351 . Bibcode :2002A&A...389..871D . doi :10.1051/0004-6361:20020668 . S2CID 18502004 . Note: see the VizieR catalogue B/ocl .
^ de La Fuente, M. R. (1998). "Dynamical Evolution of Open Star Clusters" . Publications of the Astronomical Society of the Pacific . 110 (751): 1117. Bibcode :1998PASP..110.1117D . doi :10.1086/316220 .
^ Perryman, M.A.C.; et al. (1998). "The Hyades: distance, structure, dynamics, and age". Astronomy & Astrophysics . 331 : 81– 120. arXiv :astro-ph/9707253 . Bibcode :1998A&A...331...81P .
^ Casewell, S. L.; Jameson, R. F.; Dobbie, P. D. (January 2006). "New stellar members of the Coma Berenices open star cluster" . Monthly Notices of the Royal Astronomical Society . 365 (2): 447– 453. arXiv :astro-ph/0510133 . Bibcode :2006MNRAS.365..447C . doi :10.1111/j.1365-2966.2005.09689.x .
^
Reid, M. J.; et al. (2009). "Trigonometric Parallaxes of Massive Star Forming Regions: VI. Galactic Structure, Fundamental Parameters and Non-Circular Motions". Astrophysical Journal . 700 (1): 137– 148. arXiv :0902.3913 . Bibcode :2009ApJ...700..137R . doi :10.1088/0004-637X/700/1/137 . S2CID 11347166 .
^ a b c d e f g h i j Robichon, N.; et al. (2005). "Open clusters with Hipparcos. I. Mean astrometric parameters". Astronomy and Astrophysics . 345 : 471– 484. arXiv :astro-ph/9903131 . Bibcode :1999A&A...345..471R .
^ a b c d e f g h i j k l m n o p q r s t u v w x Meynet, G.; Mermilliod, J.-C.; Maeder, A. (May 1993). "New dating of galactic open clusters". Astronomy and Astrophysics Supplement Series . 98 (3): 477– 504. Bibcode :1993A&AS...98..477M .
^ Paunzen, E.; Pintado, O. I.; Maitzen, H. M. (December 2003). "CCD photometric search for peculiar stars in open clusters. V. NGC 2099, NGC 3114, NGC 6204, NGC 6705 and NGC 6756". Astronomy and Astrophysics . 412 (3): 721– 725. arXiv :astro-ph/0310069 . Bibcode :2003A&A...412..721P . doi :10.1051/0004-6361:20031065 . S2CID 6381138 .
^ a b Kalirai, Jasonjot Singh; Fahlman, Gregory G.; Richer, Harvey B.; Ventura, Paolo (September 2003). "The CFHT Open Star Cluster Survey. IV. Two Rich, Young Open Star Clusters: NGC 2168 (M35) and NGC 2323 (M50)". The Astronomical Journal . 126 (3): 1402– 1414. arXiv :astro-ph/0306241 . Bibcode :2003AJ....126.1402K . doi :10.1086/377320 . S2CID 17018911 .
^ Pinfield, D. J.; et al. (July 2003). "Brown dwarfs and low-mass stars in the Pleiades and Praesepe: membership and binarity" . Monthly Notices of the Royal Astronomical Society . 342 (4): 1241– 1259. arXiv :astro-ph/0303600 . Bibcode :2003MNRAS.342.1241P . doi :10.1046/j.1365-8711.2003.06630.x . S2CID 285922 .
^ "NGC 2632" . sim-id . Retrieved 2020-06-11 .
^ Percival, S. M.; Salaris, M.; Groenewegen, M. A. T. (2005). "The distance to the Pleiades. Main sequence fitting in the near infrared". Astronomy and Astrophysics . 429 (3): 887– 894. arXiv :astro-ph/0409362 . Bibcode :2005A&A...429..887P . doi :10.1051/0004-6361:20041694 . S2CID 14842664 .
^ Sanner, J.; et al. (September 1999). "Photometric and kinematic studies of open star clusters. I. NGC 581 (M 103)". Astronomy and Astrophysics . 349 : 448– 456. arXiv :astro-ph/9908059 . Bibcode :1999A&A...349..448S .
^ a b c Mermilliod, J.-C.; Turon, C.; Robichon, N.; Arenou, F.; Lebreton, Y. (May 13–16, 1997). "The Distance of the Pleiades and Nearby Clusters". Proceedings of the ESA Symposium 'Hipparcos - Venice '97' . Venice, Italy: ESA. Bibcode :1997ESASP.402..643M .
^ Hünsch, M.; Weidner, C. & Schmitt, J. H. M. M. (May 2003). "An X-ray study of the open clusters NGC 2451 A and B" . Astronomy and Astrophysics . 402 (2): 571– 586. Bibcode :2003A&A...402..571H . doi :10.1051/0004-6361:20030268 .
^ Basri, Gibor; Martín, Eduardo L. (January 1999). "The Mass and Age of Very Low Mass Members of the Open Cluster alpha Persei". The Astrophysical Journal . 510 (1): 266– 273. arXiv :astro-ph/9807145 . Bibcode :1999ApJ...510..266B . doi :10.1086/306564 . S2CID 2562718 .
^ Lee, Myung Gyoon (February 1997). "UBVI CCD Photometry of the Remote Old Open Cluster AM-2" . Astronomical Journal . 113 : 729– 739. Bibcode :1997AJ....113..729L . doi :10.1086/118292 .
^ "Hodge 301" . The Hubble Heritage Project . NASA. April 1, 1999. Retrieved 2010-03-25 .
^ Grebel, Eva K.; Chu, You-Hua (February 2000). "Hubble Space Telescope Photometry of Hodge 301: An "Old" Star Cluster in 30 Doradus". The Astronomical Journal . 119 (2): 787– 799. arXiv :astro-ph/9910426 . Bibcode :2000AJ....119..787G . doi :10.1086/301218 . S2CID 118590210 .
^ "Cl Collinder 69" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2020-06-07 .
^ "Cl Collinder 135" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2020-06-07 .
^ "Cl Melotte 186" . sim-id . Retrieved 2020-07-13 .
^ "NGC 2070" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 11 August 2017 .
^ Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000). The Tycho-2 catalogue of the 2.5 million brightest stars . Vol. 355. pp. L27. Bibcode :2000A&A...355L..27H . doi :10.1888/0333750888/2862 . ISBN 978-0333750889 .
^ van Leeuwen, F. (February 2013), "Parallaxes and proper motions for 20 open clusters as based on the new Hipparcos catalogue", Astronomy and Astrophysics , 497 (1): 209– 242, arXiv :0902.1039 , Bibcode :2009A&A...497..209V , doi :10.1051/0004-6361/200811382 , S2CID 16420237 .
^ Giardino, G.; et al. (October 2008). "The X-ray luminosity of solar-mass stars in the intermediate age open cluster NGC 752". Astronomy and Astrophysics . 490 (1): 113– 123. arXiv :0808.3451 . Bibcode :2008A&A...490..113G . doi :10.1051/0004-6361:200810042 . S2CID 18980057 .
^ "Cl Collinder 121" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2020-06-07 .
^ "Cl Collinder 261" . sim-id . Retrieved 2020-06-11 .
^ Salaris, M; Weiss, A; Percival, S. M. (2004). "The age of the oldest Open Clusters" (PDF) . Astronomy & Astrophysics : 165– 167.
^ "SIMBAD Astronomical Database" . Results for NGC 2301 . Retrieved 2019-04-30 .
^ Carraro, G.; Costa, E. (March 2007). "Photometry of the five marginally studied open clusters Collinder 74, Berkeley 27, Haffner 8, NGC 2509, and VdB-Hagen 4". Astronomy and Astrophysics . 464 (2): 573– 580. arXiv :astro-ph/0611705 . Bibcode :2007A&A...464..573C . doi :10.1051/0004-6361:20066350 . S2CID 1419651 .
^ Sujatha, S.; Babu, G. S. D. (2003). "Study of open cluster NGC 2509". Bulletin of the Astronomical Society of India . 31 : 9– 18. Bibcode :2003BASI...31....9S .
^ Baxter, Eric J.; et al. (September 2009), "The Distance to NGC 2264", The Astronomical Journal , 138 (3): 963– 974, arXiv :0907.3139 , Bibcode :2009AJ....138..963B , doi :10.1088/0004-6256/138/3/963 , S2CID 7940517 .
^ Pandey, A. K.; et al. (January 2008). "Stellar contents and star formation in the young star cluster Be 59" . Monthly Notices of the Royal Astronomical Society . 383 (3): 1241– 1258. arXiv :0710.5429 . Bibcode :2008MNRAS.383.1241P . doi :10.1111/j.1365-2966.2007.12641.x . S2CID 6776240 .
^ Currie, Thayne; et al. (June 2009). "The Last Gasp of Gas Giant Planet Formation: A Spitzer Study of the 5 Myr Old Cluster NGC 2362". The Astrophysical Journal . 698 (1): 1– 27. arXiv :0903.2666 . Bibcode :2009ApJ...698....1C . doi :10.1088/0004-637X/698/1/1 . S2CID 9207187 .
^ a b Paunzen, E.; et al. (July 2006). "CCD photometric search for peculiar stars in open clusters. VII. Berkeley 11, Berkeley 94, Haffner 15, Lyngå 1, NGC 6031, NGC 6405, NGC 6834 and Ruprecht 130". Astronomy and Astrophysics . 454 (1): 171– 178. arXiv :astro-ph/0602567 . Bibcode :2006A&A...454..171P . doi :10.1051/0004-6361:20054628 . S2CID 5131254 .
^ Bonatto, C.; Bica, E.; Santos, J. F. C. Jr. (April 2005). "Spatial dependence of 2MASS luminosity and mass functions in the old open cluster NGC 188". Astronomy and Astrophysics . 433 (3): 917– 929. arXiv :astro-ph/0502453 . Bibcode :2005A&A...433..917B . doi :10.1051/0004-6361:20041113 . S2CID 5134042 .
^ Turner, David G.; et al. (September 1992). "Galactic clusters with associated Cepheid variables. II - NGC 129 and DL Cassiopeiae" . Astronomical Journal . 104 (3): 1132– 1143. Bibcode :1992AJ....104.1132T . doi :10.1086/116302 .
^ "open cluster NGC 6200" . WEBDA . Universität Wien. Retrieved 2011-10-28 .
^ Carraro, Giovanni; Chaboyer, Brian; Perencevich, James (January 2006). "The young open cluster NGC 2129" . Monthly Notices of the Royal Astronomical Society . 365 (8): 867– 873. arXiv :astro-ph/0510573 . Bibcode :2006MNRAS.365..867C . doi :10.1111/j.1365-2966.2005.09762.x . S2CID 15621721 .
^ Frinchaboy, Peter M.; et al. (2008). "Open Clusters as Galactic Disk Tracers. I. Project Motivation, Cluster Membership, and Bulk Three-Dimensional Kinematics". The Astronomical Journal . 136 (1): 118– 145. arXiv :0804.4630 . Bibcode :2008AJ....136..118F . doi :10.1088/0004-6256/136/1/118 . S2CID 16641439 . See table I, p. 12.
^ "The open cluster NGC 1980" . In the Sky . Retrieved 27 November 2017 .
^ Bonatto, C.; Bica, E. (22 October 2010). "The wide variety of evolutionary stages among 34 unstudied Teutsch open clusters" . Astronomy and Astrophysics . 521 : A74. Bibcode :2010A&A...521A..74B . doi :10.1051/0004-6361/201015222 . hdl :10183/99276 .
^ Kharchenko, N. V; Piskunov, A. E; Röser, S; Schilbach, E; Scholz, R.-D (2005). "Astrophysical parameters of Galactic open clusters". Astronomy and Astrophysics . 438 (3): 1163– 1173. arXiv :astro-ph/0501674 . Bibcode :2005A&A...438.1163K . doi :10.1051/0004-6361:20042523 . S2CID 9079873 .
Bound Unbound Visual grouping