MISCLASSIFIED
MILKY WAY
|
EC 19249-7343 | IRAS - | GSC2.4.2 SAED020973 | AAVSO - |
SIMBAD EC 19249-7343 | Pan-STARRS - | SAO - | VSX - |
GAIA DR3 6415630939116638464 | SkyMapper 193102.21-733707.6 | WRAY - | GCVS - |
2MASS J19310138-7337058 | HIP - | Hen - | BD - |
WISE J193101.98-733706.8 | 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 (°) | 292.7597Ref | Parallax (mas) | 51.687±0.092Ref | Reddening E(B-V) (mag) | 0.07±0.0Ref, Note |
Declination (°) | -73.6188Ref | Distance (kpc) | 0.02Ref, Note, 0.02Ref, Note | ||
Galactic longitude (°) | 321.4026Ref | Proper motion in α (mas/yr) | 243.19±0.08Ref | ||
Galactic latitude (°) | -28.7265Ref | Proper motion in δ (mas/yr) | -151.50±0.10Ref |
Suspected in O´Donoghue et al. (2013), based on the spectrum showing molecular bands, with the conclusion that the spectrum is similar to T CrB. The object was also included in the All-sky catalog of bright M dwarfs by Lépine & Gaidos (2011), and high proper motion and parallax from their catalog are confirmed by Gaia DR2. However, Merc et al. (2021) confirmed its non-symbiotic nature and suggested that it is either a MS-MS or MS-WD binary.