MISCLASSIFIED
MILKY WAY
|
| LAMOST J054744.99+003841.8 | IRAS 05451+0037 | GSC2.4.2 N9HL005238 | AAVSO - |
| SIMBAD IRAS 05451+0037 | Pan-STARRS 108770869374554340 | SAO - | VSX - |
| GAIA DR3 3219596240582005120 | SkyMapper - | WRAY - | GCVS - |
| 2MASS J05474500+0038418 | HIP - | Hen - | BD - |
| WISE J054744.99+003841.9 | 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 (°) | 86.9375Ref | Parallax (mas) | 2.608±0.100Ref | Reddening E(B-V) (mag) | 0.85±0.01Ref, Note |
| Declination (°) | 0.6450Ref | Distance (kpc) | 0.38Ref, Note, 0.36Ref, Note | ||
| Galactic longitude (°) | 204.9343Ref | Proper motion in α (mas/yr) | -1.81±0.10Ref | ||
| Galactic latitude (°) | -13.8276Ref | Proper motion in δ (mas/yr) | -0.63±0.08Ref |
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., Megeath et al., 2012). The Gaia data confirm main-sequence classification.