MWC 56

MISCLASSIFIED MILKY WAY
 
Constellation
Cassiopeia
Equatorial coordinates
α = 02 42 43.154
δ = +61 15 57.656
Galactic coordinates
l = 135.9004°
b = 1.2281°

Suspected 1973Ref
Re-classified 1945Ref
Type Be starRef

Identifiers

MWC 56 IRAS - GSC2.4.2 NAWM000122 AAVSO 000-BCY-883
SIMBAD EM* MWC 56 Pan-STARRS 181510406797869938 SAO - VSX 235015
GAIA DR3 465619436087728256 SkyMapper - WRAY - GCVS -
2MASS J02424317+6115575 HIP - Hen - BD -
WISE J024243.15+611557.6 TYC 4047-846-1 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 (°) 40.6798Ref Parallax (mas) 0.335±0.028Ref Reddening E(B-V) (mag) 1.09±0.09Ref, Note
Declination (°) 61.2660Ref Distance (kpc) 2.79Ref, Note, 2.75Ref, Note    
Galactic longitude (°) 135.9004Ref Proper motion in α (mas/yr) -0.09±0.03Ref    
Galactic latitude (°) 1.2281Ref Proper motion in δ (mas/yr) -0.17±0.03Ref    

Links

SIMBAD   CDS Portal


Notes

MWC 56 is included in the list of late-type emission-line stars in the paper by Allen (1973). According to the paper, these stars may be either symbiotic stars or heavily reddened objects. MWC 56 is considered the second case, specifically as a reddened Be star. We included this object in the database as the list of Allen (1973) was used by several researchers as a basis for confirming symbiotic nature.


References


Last updated: April 30, 2022