MISCLASSIFIED
MILKY WAY
|
BL Tel | IRAS 19027-5129 | GSC2.4.2 SAOX000437 | AAVSO 000-BCX-337 |
SIMBAD V* BL Tel | Pan-STARRS - | SAO 245923 | VSX 36332 |
GAIA DR3 6657628225713981312 | SkyMapper - | WRAY - | GCVS BL Tel |
2MASS J19063810-5125032 | HIP 93844 | Hen - | BD - |
WISE J190638.09-512503.1 | TYC 8386-1623-1 | ESO - | HD 177300 |
Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
Gaposchkin (1957) | BL Tel (Conf.) | Kenyon (1986) | BL Tel (Susp.) | Akras et al. (2019) | - |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | BL Tel (Conf.) |
Right ascension (°) | 286.6587Ref | Parallax (mas) | 0.566±0.030Ref | Reddening E(B-V) (mag) | 0.07±0.0Ref, Note |
Declination (°) | -51.4176Ref | Distance (kpc) | 1.68Ref, Note, 1.71Ref, Note | ||
Galactic longitude (°) | 345.5252Ref | Proper motion in α (mas/yr) | -6.15±0.02Ref | ||
Galactic latitude (°) | -23.1553Ref | Proper motion in δ (mas/yr) | 0.15±0.02Ref |
Included in the books by Gaposchkin (1957) and Kenyon (1986) in the list of suspected symbiotics. Kenyon (1986) argues that the system is similar to AR Pav, however, it consists of an M giant and an F supergiant (e.g., Feast, 1967; van Genderen et al., 1974).