MISCLASSIFIED
MILKY WAY
|
| V357 CMa | IRAS 07178-1925 | GSC2.4.2 S3SJ001131 | AAVSO 000-BCZ-560 |
| SIMBAD V* V357 CMa | Pan-STARRS 84581100169725282 | SAO - | VSX 136358 |
| GAIA DR3 2930514876802398080 | SkyMapper 072004.06-193045.3 | WRAY - | GCVS V0357 CMa |
| 2MASS J07200406-1930453 | HIP - | Hen - | BD -19 1821 |
| WISE J072004.08-193045.2 | TYC 5974-572-1 | ESO - | HD - |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | NSV 3539 (Susp.) |
| Right ascension (°) | 110.0169Ref | Parallax (mas) | 0.476±0.025Ref | Reddening E(B-V) (mag) | 0.6±0.03Ref, Note |
| Declination (°) | -19.5126Ref | Distance (kpc) | 1.99Ref, Note, 2.04Ref, Note | ||
| Galactic longitude (°) | 233.4939Ref | Proper motion in α (mas/yr) | -1.66±0.02Ref | ||
| Galactic latitude (°) | -2.7389Ref | Proper motion in δ (mas/yr) | 1.64±0.02Ref |
Suspected in Vaidis (1988). The spectrum reported by Sanduleak & Stephenson (1973) showed OB-like continuum in the ultraviolet and TiO bands with no emission lines in the blue-green region. In Pereira et al. (2003), only Hα, Hβ, and Hγ emission lines were detected, leading to the conclusion that the spectrum is similar to VV Cep. They suggested M1 I classification for the object. Classified as a Mira variable in SIMBAD (Wenger et al., 2000) with reference to GCVS, but there the star is classified as an SRa variable.