Ma 250

MISCLASSIFIED SMC
 
Constellation
Tucana
Equatorial coordinates
α = 00 48 42.952
δ = -73 03 11.348
Galactic coordinates
l = 303.2080°
b = -44.0736°

Suspected 2002Ref
Re-classified 2003Ref
Type Be starRef

Identifiers

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 -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) - Belzcyński et al. (2001) -
Gaposchkin (1957) - Kenyon (1986) - Akras et al. (2019) -
Boyarchuk (1969) - Vaidis (1988, 1991) -

Position

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
   
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    

Links

SIMBAD   CDS Portal


Notes

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.


References


Last updated: May 2, 2022