MISCLASSIFIED
MILKY WAY
|
| Hen 3-1179 | IRAS - | GSC2.4.2 S8S0000032 | AAVSO - |
| SIMBAD MR 59 | Pan-STARRS - | SAO - | VSX 2226185 |
| GAIA DR3 6021772125857703168 | SkyMapper 162003.00-363815.3 | WRAY 15-1457 | GCVS - |
| 2MASS J16200300-3638152 | HIP - | Hen 3-1179 | BD - |
| WISE J162003.00-363815.3 | 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 (°) | 245.0125Ref | Parallax (mas) | 0.071±0.023Ref | Reddening E(B-V) (mag) | 0.82±0.02Ref, Note |
| Declination (°) | -36.6376Ref | Distance (kpc) | 10.63Ref, Note, 10.18Ref, Note | ||
| Galactic longitude (°) | 342.9148Ref | Proper motion in α (mas/yr) | -3.87±0.03Ref | ||
| Galactic latitude (°) | 9.5589Ref | Proper motion in δ (mas/yr) | -1.34±0.02Ref |
Classified as a symbiotic candidate in SIMBAD (Wenger et al., 2000) with reference to Smith (1968). However, the mentioned article lists the star as a Be? object. It has also been classified as a WR star by Roberts (1962), a possible T Tau star by Henize (1976), and an M-type star with emission lines by Sanduleak & Stephenson (1973). Pereira et al. (2003) identified the star as an M supergiant (M0-M1 I).