MISCLASSIFIED
MILKY WAY
|
LAMOST J042959.50+243307.8 | IRAS - | GSC2.4.2 N9QE002945 | AAVSO - |
SIMBAD CRTS J042959.5+243307 | Pan-STARRS 137460674980173100 | SAO - | VSX - |
GAIA DR3 146366442430208640 | SkyMapper - | WRAY - | GCVS - |
2MASS J04295950+2433078 | HIP - | Hen - | BD - |
WISE J042959.50+243307.5 | 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 (°) | 67.4980Ref | Parallax (mas) | 7.589±0.120Ref | Reddening E(B-V) (mag) | 1.3±0.09Ref, Note |
Declination (°) | 24.5520Ref | Distance (kpc) | 0.13Ref, Note, 0.13Ref, Note | ||
Galactic longitude (°) | 173.5073Ref | Proper motion in α (mas/yr) | 8.51±0.17Ref | ||
Galactic latitude (°) | -16.2020Ref | Proper motion in δ (mas/yr) | -21.35±0.12Ref |
Suspected of having a symbiotic nature by Jia et al. (2023) based on the machine-learning search. The spectra from the SDSS survey suggest an accreting-only nature. However, the object was previously classified as a YSO (e.g., Luhman et al., 2006). The Gaia data confirm main-sequence classification.