MISCLASSIFIED
MILKY WAY
|
2MASS J07363415+6538548 | IRAS - | GSC2.4.2 N7TR013962 | AAVSO - |
SIMBAD UCAC4 779-021043 | Pan-STARRS 186771141422129050 | SAO - | VSX 2203990 |
GAIA DR3 1089778926942542592 | SkyMapper - | WRAY - | GCVS - |
2MASS J07363415+6538548 | HIP - | Hen - | BD - |
WISE J073634.15+653854.8 | 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 (°) | 114.1422Ref | Parallax (mas) | 2.427±0.038Ref | Reddening E(B-V) (mag) | 0.03±0.0Ref, Note |
Declination (°) | 65.6486Ref | Distance (kpc) | 0.41Ref, Note, 0.40Ref, Note | ||
Galactic longitude (°) | 150.5153Ref | Proper motion in α (mas/yr) | -2.55±0.02Ref | ||
Galactic latitude (°) | 29.1577Ref | Proper motion in δ (mas/yr) | 6.04±0.03Ref |
Discovered as an X-ray source in the NGC2403 field by Schlegel & Pannuti (2003). Binder et al. (2015) noticed properties similar to an NS accreting from the wind of a late-type giant (e.g., symbiotic star GX 1+4). Rapid X-ray variability was observed. Merc et al. (2020) analyzed multifrequency observations of the object, together with the photometric variability and concluded that the star is an active foreground K-type dwarf. Spectroscopic observations of Dubovský et al. (2021) confirmed the classification.