astro.wikisort.org - StarBerkeley 87 is an open cluster in a heavily obscured region of the Milky Way in Cygnus.[2] The rare WO type Wolf–Rayet star WR 142 is a member of Berkeley 87.[3]
Berkeley 87 |
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Constellation | Cygnus |
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Right ascension | 20h 21m 43.01s[1] |
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Declination | +37° 22′ 13.8″[1] |
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Distance | ~1650 pc |
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Apparent dimensions (V) | 8 |
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Other designations | Dolidze 7, OCl 161, C 2019+372, OCISM 34, MWSC 3325 |
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See also: Open cluster, List of open clusters |
This cluster contains HD 229059 which, as of August 2021, is the nearest known star to Earth with a Bolometric Luminosity greater than 1 million L☉.[4]
Prominent stars[5]
Star name |
Effective temperature |
Absolute magnitude |
Bolometric magnitude |
Mass (M☉) |
Spectral type |
WR 142 (Berkeley 87–29) |
200000 K |
-3.13 |
-10.1 |
28.6 |
WO2 |
HD 229059 (Berkeley 87–3) |
26300 K |
-7.7 |
-10.3 |
69 |
B1Ia |
Berkeley 87-25 |
35700 K |
-5.6 |
-9.1 |
39 |
O8.5III |
Berkeley 87-15 |
37800 K |
-5 |
-8.6 |
34 |
B[e] |
Berkeley 87-4 |
29500 K |
-5 |
-7.9 |
23 |
B0.2III |
References
- "Berkeley 87". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 31 December 2020.
- Turner, D. G.; Forbes, D. (1982). "Berkeley 87, a heavily-obscured young cluster associated with the ON2star-formation complex and containing the WO star Stephenson 3". Publications of the Astronomical Society of the Pacific. 94: 789–801. Bibcode:1982PASP...94..789T. doi:10.1086/131065.
- Sokal, Kimberly R.; Skinner, Stephen L.; Zhekov, Svetozar A.; Güdel, Manuel; Schmutz, Werner (2010). "Chandra Detects the Rare Oxygen-type Wolf-Rayet Star WR 142 and OB Stars in Berkeley 87". The Astrophysical Journal. 715 (2): 1327–1337. arXiv:1004.0462. Bibcode:2010ApJ...715.1327S. doi:10.1088/0004-637X/715/2/1327. S2CID 119232391.
- "List of most luminous stars".
- Massey, P.; Degioia-Eastwood, K.; Waterhouse, E. (2001). "The Progenitor Masses of Wolf-Rayet Stars and Luminous Blue Variables Determined from Cluster Turnoffs. II. Results from 12 Galactic Clusters and OB Associations". The Astronomical Journal. 121 (2): 1050–1070. arXiv:astro-ph/0010654. Bibcode:2001AJ....121.1050M. doi:10.1086/318769. S2CID 53345173.
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