NGC 371, also called Hodge 53, is an open cluster 200,000 light-years (61,320 pc) away located in the Small Magellanic Cloud in Tucana constellation. It was discovered on 1 August 1826 by Scottish astronomer James Dunlop.[2]
Prominent stars[3][4]
Star name
|
Effective temperature (K)
|
Absolute magnitude
|
Bolometric magnitude
|
Mass (M☉)
|
Spectral type
|
AB6
|
105000/35000
|
-5.15/-6.65
|
-10.96/-10.01
|
9/41
|
WN4+O6.5I
|
AB7
|
105000/36000
|
-4.4/-5.7
|
-10.51/-9.01
|
23/44
|
WN4+O6I(f)
|
Hodge53-207
|
50100
|
-4.8
|
-9.3
|
53
|
O
|
Hodge53-47a
|
48600
|
-4.9
|
-9.3
|
50
|
O4V
|
Hodge53-47b
|
42400
|
-4.9
|
-8.9
|
37
|
O6.5V
|
Hodge53-60
|
37200
|
-5.4
|
-9
|
36
|
O8III
|
AV 327
|
33000
|
-5.8
|
-9.1
|
35
|
O9I
|
Hodge53-141
|
34400
|
-5.8
|
-9.2
|
34
|
O9III
|
Hodge53-137
|
35700
|
-5.6
|
-9.1
|
34
|
O8.5III
|
Hodge53-118
|
42500
|
-4.6
|
-8.6
|
34
|
|
Hodge53-91
|
37200
|
-5.1
|
-8.7
|
32
|
O8.5V
|
Hodge53-11
|
41800
|
-4.4
|
-8.3
|
31
|
|
Hodge53-74
|
39400
|
-4.6
|
-8.4
|
30
|
|
See also
References
- ^ "NGC 371". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2010-03-31.
- ^ Seligman, Courtney. "New General Catalogue Objects: NGC 371". Celestial Atlas. Retrieved 29 August 2024.
- ^ Massey, Philip; Waterhouse, Elizabeth; DeGioia-Eastwood, Kathleen (May 2000). "The Progenitor Masses of Wolf-Rayet Stars and Luminous Blue Variables Determined from Cluster Turnoffs. I. Results from 19 OB Associations in the Magellanic Clouds". The Astronomical Journal. 119 (5): 2214–2241. arXiv:astro-ph/0002233. Bibcode:2000AJ....119.2214M. doi:10.1086/301345. ISSN 0004-6256. S2CID 16891188.
- ^ Shenar, T.; Hainich, R.; Todt, H.; Sander, A.; Hamann, W.-R.; Moffat, A. F. J.; Eldridge, J. J.; Pablo, H.; Oskinova, L. M.; Richardson, N. D. (2016). "Wolf-Rayet stars in the Small Magellanic Cloud: II. Analysis of the binaries". Astronomy & Astrophysics. 1604: A22. arXiv:1604.01022. Bibcode:2016A&A...591A..22S. doi:10.1051/0004-6361/201527916. S2CID 119255408.
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