W Cephei

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W Cephei
Observation data
Epoch 2000      Equinox 2000
Constellation Cepheus
Right ascension 22h 36m 27.56359s[1]
Declination +58° 25′ 343.9456″[1]
Apparent magnitude (V) 7.02 - 9.20[2]
Characteristics
Spectral type K0ep-M2ep Ia + B0/B1[2]
Variable type SRc[2]
Astrometry
Radial velocity (Rv) −44.64[3] km/s
Proper motion (μ) RA: −2.48[1] mas/yr
Dec.: −3.27[1] mas/yr
Parallax (π) 0.02 ± 0.59[1] mas
Distance 2,427[4] pc
Absolute magnitude (MV) −7[5] + −3.5[6]
Details[7]
Luminosity 72,400 L
Temperature 4,400 K
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.[4][8]

Discovery

W Cephei was reported in 1896 as a red star varying from magnitude 7.3 to 8.3.[9] It was catalogued as BD+57°2568 in the Bonner Durchmusterung published in 1903, and HD 214369 in the Henry Draper Catalogue.

In 1925, W Cep was included in a listing of Be stars. It was recognised as a cool star with spectral type Mep.[10] It was classified as K0ep Ia from a 1949 spectrum, but also recognised to have a small hot companion, plus an unusual infrared excess.[11][12] Ultraviolet spectra allowed absorption lines from the companion to be studied and it was given a spectral type of B0-1.[13]

System

The W Cephei system contains a K class 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.[5] The two components have been resolved at 0.262" using Speckle interferometry.[14] An orbital period of 2,090 days has been proposed.[8]

Variability

W Cephei varies in brightness from 7th to 9th magnitude. The General Catalogue of Variable Stars lists it as a semiregular variable but attempts to find a period have shown only random variations.[15][16]

References

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External links

Coordinates: Sky map 22h 36m 27.60s, +58° 25′ 34.0″