MISCLASSIFIED
MILKY WAY
|
LAMOST J094254.61+315049.2 | IRAS - | GSC2.4.2 N9BT023432 | AAVSO - |
SIMBAD SDSS J094254.50+315103.5 | Pan-STARRS 146211457274967043 | SAO - | VSX - |
GAIA DR3 793037643597158016 | SkyMapper - | WRAY - | GCVS - |
2MASS - | HIP - | Hen - | BD - |
WISE - | 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 (°) | 145.7276Ref | Parallax (mas) | -0.649±0.700Ref | Reddening E(B-V) (mag) | 0.02±0.0Ref, Note |
Declination (°) | 31.8469Ref | Distance (kpc) | 2.67Ref, Note, 5.46Ref, Note | ||
Galactic longitude (°) | 194.6162Ref | Proper motion in α (mas/yr) | 0.70±0.69Ref | ||
Galactic latitude (°) | 49.0188Ref | Proper motion in δ (mas/yr) | 2.46±0.46Ref |
Suspected of having a symbiotic nature by Jia et al. (2023) based on the machine-learning search. However, the authors noted that the spectra from LAMOST and SDSS surveys classified the source as a galaxy. The images of the source indicate the galaxy as well.