MISCLASSIFIED
MILKY WAY
|
V549 Vel | IRAS - | GSC2.4.2 S66I023561 | AAVSO 000-BML-068 |
SIMBAD V* V549 Vel | Pan-STARRS - | SAO - | VSX 545313 |
GAIA DR3 5328722978788574080 | SkyMapper 085029.64-474527.9 | WRAY - | GCVS V0549 Vel |
2MASS J08502962-4745283 | HIP - | Hen - | BD - |
WISE J085029.64-474527.9 | 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 (°) | 132.6234Ref | Parallax (mas) | 0.934±0.286Ref | Reddening E(B-V) (mag) | 0.96±0.04Ref, Note |
Declination (°) | -47.7578Ref | Distance (kpc) | 1.70Ref, Note, 1.32Ref, Note | ||
Galactic longitude (°) | 267.1953Ref | Proper motion in α (mas/yr) | -2.78±0.34Ref | ||
Galactic latitude (°) | -2.3242Ref | Proper motion in δ (mas/yr) | 5.88±0.31Ref |
Detected in an outburst in 2017, this object may be the least luminous γ-ray nova observed so far or a symbiotic system, depending on the distance (Li et al., 2020). Later, an orbital period of 0.4 days was detected by Schaefer (2021).