MISCLASSIFIED
M33
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Object X | IRAS - | GSC2.4.2 NBWQ019086 | AAVSO - |
SIMBAD 2MASS J01332404+3025345 | Pan-STARRS 144510233487992335 | SAO - | VSX - |
GAIA DR3 303270801867223936 | SkyMapper - | WRAY - | GCVS - |
2MASS J01332404+3025345 | HIP - | Hen - | BD - |
WISE J013324.03+302534.5 | 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 (°) | 23.3488Ref | Parallax (mas) | 0.396±0.616Ref | Reddening E(B-V) (mag) | 0.04±0.0Ref, Note |
Declination (°) | 30.4264Ref | Distance (kpc) | 847±60Ref 1.31Ref, Note -, Note |
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Galactic longitude (°) | 133.5503Ref | Proper motion in α (mas/yr) | -0.18±0.67Ref | ||
Galactic latitude (°) | -31.5788Ref | Proper motion in δ (mas/yr) | -0.53±0.48Ref |
Object X is identified as the most luminous infrared star in M33, characterized by a composite nature with a hot, luminous O-B star component and a cool, dust-enshrouded companion. Described as a very young and massive binary star, it was referred to as a "super symbiotic binary" in Mikołajewska et al. (2015). However, it is noted that it does not fulfill the criteria for symbiotic binaries, leading to a classification as a related object, but not a symbiotic star.