MISCLASSIFIED
MILKY WAY
|
V976 Aql | IRAS 19279+1117 | GSC2.4.2 N2A9042813 | AAVSO 000-BDF-349 |
SIMBAD V* V976 Aql | Pan-STARRS 121672925772582198 | SAO - | VSX 2115 |
GAIA DR3 4314928315484576256 | SkyMapper - | WRAY - | GCVS V0976 Aql |
2MASS J19301855+1123353 | HIP - | Hen - | BD - |
WISE J193018.53+112335.4 | TYC - | 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 (°) | 292.5773Ref | Parallax (mas) | 0.245±0.082Ref | Reddening E(B-V) (mag) | 0.86±0.02Ref, Note |
Declination (°) | 11.3931Ref | Distance (kpc) | 4.52Ref, Note, 5.11Ref, Note | ||
Galactic longitude (°) | 47.5084Ref | Proper motion in α (mas/yr) | 0.08±0.07Ref | ||
Galactic latitude (°) | -3.2786Ref | Proper motion in δ (mas/yr) | -3.59±0.06Ref |
Mentioned as a symbiotic star by Bond (1976), with reference to Allen (1974). The latter classified the object as a compact PN resembling a late-type star (his class S). He also claimed that most objects in this class are symbiotics or VV Cep-type stars. It was later classified as a Mira variable (Geßner, 1983) and a late-type star by Acker et al. (1987).