Region around γ Cygni, with RW Cygni annotated on the full-size image (north is right)
Observation data Epoch J2000 Equinox J2000
Constellation
Cygnus
Right ascension
20h 28m 50.59027s[1]
Declination
39° 58′ 54.4180″[1]
Apparent magnitude (V)
8.05 - 9.70[2]
Characteristics
Evolutionary stage
Red supergiant
Spectral type
M3-4Ia-Iab[3]
Variable type
SRc[2]
Astrometry
Radial velocity (Rv)
−18.39±0.52[1] km/s
Proper motion (μ)
RA: –3.255[1] mas/yr Dec.: –5.511[1] mas/yr
Parallax (π)
0.4602 ± 0.0897 mas[1]
Distance
1,620±40[4] pc
Absolute magnitude (MV)
–6.41[5]
Details
Radius
1103+251 −177[6]R☉
Luminosity
126,000[4]L☉
Temperature
3,600[7] K
Other designations
RW Cyg, BD+39 4208, HIP 101023, IRAS 20270+3948, 2MASS J20285059+3958543
Database references
SIMBAD
data
RW Cygni is a semiregular variable star in the constellation Cygnus, about a degree east of 2nd magnitude γ Cygni. Its apparent magnitude varies between 8.05 and 9.70 and its spectral type between M3 and M4.
^ abcdefBrown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
^ abSamus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S.
^Keenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins catalog of revised MK types for the cooler stars". Astrophysical Journal Supplement Series. 71: 245. Bibcode:1989ApJS...71..245K. doi:10.1086/191373. S2CID 123149047.
^ abDavies, Ben; Beasor, Emma R. (March 2020). "The 'red supergiant problem': the upper luminosity boundary of Type II supernova progenitors". MNRAS. 493 (1): 468–476. arXiv:2001.06020. Bibcode:2020MNRAS.493..468D. doi:10.1093/mnras/staa174. S2CID 210714093.
^Levesque, Emily M.; Massey, Philip; Olsen, K. A. G.; Plez, Bertrand; Josselin, Eric; Maeder, Andre; Meynet, Georges (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. S2CID 15109583.
^Norris, Ryan (2021-03-01). An Interferometric Imaging Survey of Red Supergiant Stars. Bibcode:2021csss.confE.263N. doi:10.5281/zenodo.4567641.
^Norris, Ryan P. (2019). Seeing Stars Like Never Before: A Long-term Interferometric Imaging Survey of Red Supergiants(PDF) (PhD). Georgia State University.
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