NR Vulpeculae
Appearance
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Vulpecula |
Right ascension | 19h 50m 11.9270s[1] |
Declination | 24° 55′ 24.183″[1] |
Apparent magnitude (V) | 9.13 - 9.61[2] |
Characteristics | |
Spectral type | M1Ia[2] |
Variable type | LC[2] |
Astrometry | |
Proper motion (μ) | RA: −1.435[1] mas/yr Dec.: −6.223[1] mas/yr |
Parallax (π) | −0.08 ± 0.63 mas[1] |
Details | |
Radius | 980[3] R☉ |
Luminosity | 225,000[3] L☉ |
Temperature | 4,000[3] K |
Other designations | |
Database references | |
SIMBAD | data |
NR Vulpeculae is a red supergiant and irregular variable star in the constellation Vulpecula. It is one of the largest known stars.
References
- ^ a b c d e Gaia Collaboration; Brown, A. G. A.; Vallenari, A.; Prusti, T.; De Bruijne, J. H. J.; Mignard, F.; Drimmel, R.; Babusiaux, C.; Bailer-Jones, C. A. L.; Bastian, U.; Biermann, M.; Evans, D. W.; Eyer, L.; Jansen, F.; Jordi, C.; Katz, D.; Klioner, S. A.; Lammers, U.; Lindegren, L.; Luri, X.; O'Mullane, W.; Panem, C.; Pourbaix, D.; Randich, S.; Sartoretti, P.; Siddiqui, H. I.; Soubiran, C.; Valette, V.; Van Leeuwen, F.; et al. (2016). "Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties". Astronomy & Astrophysics. 595: A2. Bibcode:2016A&A...595A...2G. doi:10.1051/0004-6361/201629512.
- ^ a b c NR Vul, database entry, The combined table of GCVS Vols I-III and NL 67-78 with improved coordinates, General Catalogue of Variable Stars, Sternberg Astronomical Institute, Moscow, Russia. Accessed on line November 12, 2010.
- ^ a b c Levesque, Emily M.; Massey, Philip; Olsen, K. A. G.; Plez, Bertrand; Josselin, Eric; Maeder, Andre; Meynet, Georges (August 2005). "The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not As Cool As We Thought". The Astrophysical Journal. 628 (2): 973–985. arXiv:astro-ph/0504337. Bibcode:2005ApJ...628..973L. doi:10.1086/430901.