MISCLASSIFIED
SMC
|
Ma 250 | IRAS - | GSC2.4.2 S0XH458606 | AAVSO - |
SIMBAD [MA93] 250 | Pan-STARRS - | SAO - | VSX - |
GAIA DR3 4685950607187395584 | SkyMapper 004842.95-730311.4 | WRAY - | GCVS - |
2MASS J00484294-7303113 | HIP - | Hen - | BD - |
WISE J004842.93-730311.3 | 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 (°) | 12.1790Ref | Parallax (mas) | -0.046±0.035Ref | Reddening E(B-V) (mag) | 0.88±0.22Ref, Note |
Declination (°) | -73.0532Ref | Distance (kpc) | 62.1±1.9Ref 18.52Ref, Note, 13.27Ref, Note |
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Galactic longitude (°) | 303.2080Ref | Proper motion in α (mas/yr) | 0.64±0.05Ref | ||
Galactic latitude (°) | -44.0736Ref | Proper motion in δ (mas/yr) | -1.17±0.04Ref |
Included in the list of possible symbiotic stars or closely related objects in Munari & Zwitter (2002), the spectrum of this object shows Balmer lines in emission and a flat continuum. In Cieslinski et al. (2013), the object was classified as a Be star. In Pawlak et al. (2016), the star was classified as an eclipsing binary with a period of 58.4 days.