MISCLASSIFIED
MILKY WAY
|
V630 Cas | IRAS - | GSC2.4.2 N18B032196 | AAVSO 000-BCS-001 |
SIMBAD V* V630 Cas | Pan-STARRS 169753572163253716 | SAO - | VSX 6961 |
GAIA DR3 1944248097659113088 | SkyMapper - | WRAY - | GCVS V0630 Cas |
2MASS J23485191+5127391 | HIP - | Hen - | BD - |
WISE J234851.91+512739.0 | TYC - | ESO - | HD - |
Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
Right ascension (°) | 357.2163Ref | Parallax (mas) | 0.381±0.037Ref | Reddening E(B-V) (mag) | 0.19±0.0Ref, Note |
Declination (°) | 51.4609Ref | Distance (kpc) | 2.41Ref, Note, 2.54Ref, Note | ||
Galactic longitude (°) | 113.1030Ref | Proper motion in α (mas/yr) | -0.86±0.03Ref | ||
Galactic latitude (°) | -10.2128Ref | Proper motion in δ (mas/yr) | -4.10±0.03Ref |
Listed among possible symbiotic stars or closely related objects in Munari & Zwitter (2002), this star's spectrum, despite having very low signal-to-noise ratio, exhibits Hα emission. Orosz et al. (2001) classified the same star as a dwarf nova and determined an orbital period of 2.56 days.