MISCLASSIFIED
MILKY WAY
|
WRAY 15-1423 | IRAS - | GSC2.4.2 S8UK064183 | AAVSO - |
SIMBAD WRAY 15-1423 | Pan-STARRS - | SAO - | VSX 58959 |
GAIA DR3 5993545914349355264 | SkyMapper 160912.25-414025.3 | WRAY 15-1423 | GCVS - |
2MASS J16091226-4140249 | HIP - | Hen 3-1146 | BD - |
WISE J160912.26-414025.2 | TYC - | ESO - | HD - |
Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | Sz 134 (Susp.) |
Right ascension (°) | 242.3011Ref | Parallax (mas) | 6.433±0.022Ref | Reddening E(B-V) (mag) | 0.62±0.01Ref, Note |
Declination (°) | -41.6737Ref | Distance (kpc) | 0.15Ref, Note, 0.15Ref, Note | ||
Galactic longitude (°) | 337.8407Ref | Proper motion in α (mas/yr) | -10.06±0.03Ref | ||
Galactic latitude (°) | 7.4159Ref | Proper motion in δ (mas/yr) | -27.56±0.02Ref |
Suspected by Vaidis (1988). Previously classified as Mep? by Sanduleak & Stephenson (1973), and as a probable T Tauri star by Henize (1976). Weak TiO absorption, along with Balmer lines in emission, was detected by Allen (1978). Additionally, He I lines in emission were observed by Schwartz & Noah (1978). In Pereira et al. (2003), it was noted that the continuum spectrum resembles that of known T Tau stars, with the detection of He II in emission. Dwarf classification is further supported by the Gaia distance.