MISCLASSIFIED
MILKY WAY
|
Hen 3-814 | IRAS 12413-6139 | GSC2.4.2 S7LF000534 | AAVSO 000-BGY-203 |
SIMBAD CD-61 3575 | Pan-STARRS - | SAO - | VSX 95424 |
GAIA DR3 6055427493901807104 | SkyMapper 124416.17-615621.2 | WRAY - | GCVS - |
2MASS J12441615-6156209 | HIP - | Hen 3-814 | BD - |
WISE J124416.16-615621.2 | TYC 8992-314-1 | 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 (°) | 191.0672Ref | Parallax (mas) | 0.460±0.036Ref | Reddening E(B-V) (mag) | 6.57±1.23Ref, Note |
Declination (°) | -61.9392Ref | Distance (kpc) | 2.08Ref, Note, 2.07Ref, Note | ||
Galactic longitude (°) | 302.0888Ref | Proper motion in α (mas/yr) | -4.70±0.03Ref | ||
Galactic latitude (°) | 0.9208Ref | Proper motion in δ (mas/yr) | -0.45±0.04Ref |
Listed as a confirmed symbiotic binary in SIMBAD (Wenger et al., 2000), with the reference to Henize (1976). However, Henize (1976) suggested a possible VV Cephei type classification. Pereira et al. (2003) supported such classification as they classified the object as an M2 I star. The confirmation of an Ia class star through absolute infrared magnitude measurements is reported by Munari et al. (2021).