MISCLASSIFIED
MILKY WAY
|
W Cep | IRAS 22345+5809 | GSC2.4.2 N1C7000418 | AAVSO 000-BCQ-570 |
SIMBAD V* W Cep | Pan-STARRS 178113391148011769 | SAO 34614 | VSX 8358 |
GAIA DR3 2008330491486269440 | SkyMapper - | WRAY - | GCVS W Cep |
2MASS J22362757+5825340 | HIP 111592 | Hen - | BD +57 2568 |
WISE J223627.55+582533.9 | TYC 3995-937-1 | ESO - | HD 214369 |
Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
Gaposchkin (1957) | W Cep (Conf.) | Kenyon (1986) | - | Akras et al. (2019) | - |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | W Cep (Susp.) |
Right ascension (°) | 339.1148Ref | Parallax (mas) | 0.028±0.035Ref | Reddening E(B-V) (mag) | 1.51±0.08Ref, Note |
Declination (°) | 58.4261Ref | Distance (kpc) | 9.75Ref, Note, 9.39Ref, Note | ||
Galactic longitude (°) | 106.0228Ref | Proper motion in α (mas/yr) | -3.18±0.04Ref | ||
Galactic latitude (°) | 0.0571Ref | Proper motion in δ (mas/yr) | -2.28±0.03Ref |
Included in the list of symbiotic candidates by Vaidis (1988), likely due to Gaposchkin (1957) mentioning the object as a symbiotic star as noted by Garcia (1986). However, it is identified as a VV Cephei type star (Cowley, 1969). The presence of a red supergiant with a B-type companion was subsequently confirmed by Neugent et al. (2018).