Astronomy:BD+60°2522
 NGC 7635 surrounding BD+60 2522 Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA) | |
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Cassiopeia |
| Right ascension | 23h 20m 44.5135s[1] |
| Declination | +61° 11′ 40.531″[1] |
| Apparent magnitude (V) | 8.67[2] |
| Characteristics | |
| Spectral type | O6.5(f)(n)p[3] |
| U−B color index | −0.62[2] |
| B−V color index | +0.41[2] |
| Astrometry | |
| Radial velocity (Rv) | −26[4] km/s |
| Proper motion (μ) | RA: −2.662[1] mas/yr Dec.: 0.388[1] mas/yr |
| Parallax (π) | 0.3341 ± 0.0152[1] mas |
| Distance | 9,800 ± 400 ly (3,000 ± 100 pc) |
| Absolute magnitude (MV) | −5.5[5] |
| Details[6] | |
| Mass | 44 M☉ |
| Radius | 15 R☉ |
| Luminosity | 398,000 L☉ |
| Temperature | 37,500 K |
| Rotational velocity (v sin i) | 178 - 240 km/s |
| Age | 2[7] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
BD+60°2522 is a bright O-type star that has produced the Bubble Nebula (NGC 7635) with its stellar wind. The exact classification of the star is uncertain, with a number of spectral peculiarities and inconsistencies between the appearance of the star itself and the effects on the nearby nebulosity, but it is undoubtedly a highly luminous hot massive star.[5] Direct spectroscopy yields a spectral class of O6.5 and an effective temperature around 37,500 K. It is a member of the Cassiopeia OB2 stellar association in the Perseus Arm[7] of the galaxy at about 8,500 light-years' distance.[8]
Although BD+60°2522 is around two million years old, the surrounding nebula is apparently only about 40,000 years old. The bubble is expected to be formed as a shock front where the stellar wind meets interstellar material at supersonic speeds. The wind from BD+60°2522 is travelling outwards at 1,800–2,500 km/s, causing the star to lose over a millionth of the mass of the Sun every year.[7]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940 Gaia DR3 record for this source at VizieR.
- ↑ 2.0 2.1 2.2 Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues 2237. Bibcode: 2002yCat.2237....0D.
- ↑ Walborn, Nolan R.; Howarth, Ian D.; Evans, Christopher J.; Crowther, Paul A.; Moffat, Anthony F. J.; St-Louis, Nicole; Fariña, Cecilia; Bosch, Guillermo L. et al. (2010). "The Onfp Class in the Magellanic Clouds". The Astronomical Journal 139 (3): 1283. doi:10.1088/0004-6256/139/3/1283. Bibcode: 2010AJ....139.1283W.
- ↑ Wilson, Ralph Elmer (1953). "General Catalogue of Stellar Radial Velocities". Carnegie Institute Washington D.C. Publication (Carnegie Institution of Washington). ISBN 9780598216885. Bibcode: 1953GCRV..C......0W.
- ↑ 5.0 5.1 Moore, B. D.; Walter, D. K.; Hester, J. J.; Scowen, P. A.; Dufour, R. J.; Buckalew, B. A. (2002). "Hubble Space Telescope Observations of the Windblown Nebula NGC 7635". The Astronomical Journal 124 (6): 3313. doi:10.1086/344596. Bibcode: 2002AJ....124.3313M.
- ↑ Rauw, G.; De Becker, M.; Vreux, J. -M. (2004). "Line profile variability in the spectra of Oef stars". Astronomy and Astrophysics 399: 287–296. doi:10.1051/0004-6361:20021776. Bibcode: 2003A&A...399..287R.
- ↑ 7.0 7.1 7.2 Anand, M. Y.; Kagali, B. A.; Murthy, Jayant (2009). "Study of Bubble nebula using IUE high resolution spectra". Bulletin of the Astronomical Society of India 37 (1): 1. Bibcode: 2009BASI...37....1A.
- ↑ Mason, Brian D.; Hartkopf, William I.; Gies, Douglas R.; Henry, Todd J.; Helsel, John W. (2009). "The High Angular Resolution Multiplicity of Massive Stars". The Astronomical Journal 137 (2): 3358. doi:10.1088/0004-6256/137/2/3358. Bibcode: 2009AJ....137.3358M.
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