MISCLASSIFIED
MILKY WAY
|
LY Mus | IRAS 13372-7136 | GSC2.4.2 S7RV000162 | AAVSO 000-BDW-070 |
SIMBAD V* LY Mus | Pan-STARRS - | SAO 257077 | VSX 19949 |
GAIA DR3 5839896036299695104 | SkyMapper 134113.53-715205.4 | WRAY - | GCVS LY Mus |
2MASS J13411359-7152056 | HIP 66783 | Hen 4-138 | BD - |
WISE J134113.50-715205.2 | TYC 9251-1340-1 | ESO - | HD 118685 |
Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
Right ascension (°) | 205.3062Ref | Parallax (mas) | 3.250±0.051Ref | Reddening E(B-V) (mag) | 0.34±0.0Ref, Note |
Declination (°) | -71.8681Ref | Distance (kpc) | 0.31Ref, Note, 0.30Ref, Note | ||
Galactic longitude (°) | 306.8300Ref | Proper motion in α (mas/yr) | -32.26±0.05Ref | ||
Galactic latitude (°) | -9.3742Ref | Proper motion in δ (mas/yr) | 36.21±0.05Ref |
Classified as a confirmed symbiotic binary in SIMBAD (Wenger et al., 2000) with the reference to Jorissen et al. (2012). The aforementioned article mentions weak Hα emission discovered by van Eck & Jorissen (2002). However, in van Eck & Jorissen (2002), the authors detected week Hα emission but claimed that it might be due to template mismatch.