MISCLASSIFIED
MILKY WAY
|
V4375 Sgr | IRAS 17450-2759 | GSC2.4.2 S8DY000140 | AAVSO 000-BCX-108 |
SIMBAD HD 316285 | Pan-STARRS 74382670583552737 | SAO 185776 | VSX 32075 |
GAIA DR3 4057682692354437888 | SkyMapper - | WRAY 15-1777 | GCVS V4375 Sgr |
2MASS J17481403-2800531 | HIP 87136 | Hen 3-1482 | BD - |
WISE J174814.01-280052.8 | TYC 6836-356-1 | ESO 455-43 | HD 316285 |
Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
Right ascension (°) | 267.0585Ref | Parallax (mas) | 0.301±0.029Ref | Reddening E(B-V) (mag) | 61.73±7.29Ref, Note |
Declination (°) | -28.0148Ref | Distance (kpc) | 2.91Ref, Note, 2.98Ref, Note | ||
Galactic longitude (°) | 1.0857Ref | Proper motion in α (mas/yr) | -2.16±0.03Ref | ||
Galactic latitude (°) | -0.0132Ref | Proper motion in δ (mas/yr) | -4.56±0.02Ref |
Noted as a possible symbiotic star already by Allen (1973), it was subsequently classified as a potential symbiotic star by Mikołajewska et al. (1997). Although its emission line spectrum bears resemblance to Be stars, the continuum slope suggests a G-type star.Hillier et al. (1998) proposed that the object is a P Cyg-type supergiant.