W Cephei
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Cepheus |
| Right ascension | 22h 36m 27.56307s[2] |
| Declination | +58° 25′ 33.9554″[2] |
| Apparent magnitude (V) | 6.83 - 9.20[3] |
| Characteristics | |
| Evolutionary stage | Red supergiant + non-supergiant B class star |
| Spectral type | K0ep-M2ep Ia + B0/B1[3] |
| Variable type | SRc[3] |
| Astrometry | |
| Radial velocity (Rv) | −44.64[4] km/s |
| Proper motion (μ) | RA: −3.176[2] mas/yr Dec.: −2.277[2] mas/yr |
| Distance | 2,427[5] pc |
| Absolute magnitude (MV) | −7[6] + −3.5[7] |
| Orbit[8] | |
| Period (P) | 2,075 d |
| Eccentricity (e) | 0.149 |
| Inclination (i) | 90° |
| Details | |
| Radius | 670+20 −10[2] R☉ |
| Luminosity | 292,000[9] L☉ |
| Surface gravity (log g) | 0.18[2] cgs |
| Temperature | 3,681[9] – 4,400[10] K |
| Metallicity | 0.0205[2] |
| Other designations | |
| W Cep, BD+57°2568, HD 214369, HIP 111592, GSC 03995-00937, SAO 34614, PPM 40864, GC 31569, UCAC3 297-183471, IRAS 22345+5809, 2MASS J22362757+5825340, AAVSO 2232+57 | |
| Database references | |
| SIMBAD | data |
W Cephei is a spectroscopic binary and variable star located in the constellation Cepheus. It is thought to be a member of the Cep OB1 stellar association at about 8,000 light years.[5][11]
Discovery
[edit | edit source]W Cephei was catalogued as BD+57°2568 in the Bonner Durchmusterung published in 1903, and HD 214369 in the Henry Draper Catalogue. It was discovered to be a variable star by T. H. E. C. Espin, in 1885.[12] It was described in 1896 as a red star varying from magnitude 7.3 to 8.3.[13]
In 1925, W Cep was included in a listing of Be stars. It was recognised as a cool star with spectral type Mep.[14] It was classified as K0ep Ia from a 1949 spectrum, but also recognised to have a small hot companion, plus an unusual infrared excess.[15][16] Ultraviolet spectra allowed absorption lines from the companion to be studied and it was given a spectral type of B0-1.[17]
System
[edit | edit source]The W Cephei system contains a luminous red supergiant star with a non-supergiant early B companion. The star has unusual emission lines including both permitted and forbidden FeII, produced by a circumstellar envelope containing dust and ionised gas.[6] The two components have been resolved at 0.262″ using speckle interferometry.[18] An orbital period of 2,090 days has been proposed.[11]
Variability
[edit | edit source]W Cephei varies in brightness from 7th to 9th magnitude. The General Catalogue of Variable Stars lists it as a semiregular variable with a period of 370 days, but later attempts to find a period have shown only random variations.[19][20] It has also been proposed that eclipses occur.[21]
References
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External links
[edit | edit source]- AAVSO chart of comparison stars for W Cephei Archived 2011-06-14 at the Wayback Machine
- British Astronomical Association VSS light curves