MISCLASSIFIED
MILKY WAY
|
PN M1-67 | IRAS 19092+1646 | GSC2.4.2 N2CZ000008 | AAVSO 000-BCW-968 |
SIMBAD - | Pan-STARRS 128232878787583130 | SAO - | VSX 27667 |
GAIA DR3 4513494205567536512 | SkyMapper - | WRAY - | GCVS QR Sge |
2MASS J19113087+1651382 | HIP 94289 | Hen - | BD - |
WISE J191130.87+165138.1 | TYC 1586-411-1 | 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 (°) | 287.8786Ref | Parallax (mas) | 0.157±0.014Ref | Reddening E(B-V) (mag) | 1.37±0.04Ref, Note |
Declination (°) | 16.8606Ref | Distance (kpc) | 5.36Ref, Note, 5.43Ref, Note | ||
Galactic longitude (°) | 50.1980Ref | Proper motion in α (mas/yr) | -2.52±0.01Ref | ||
Galactic latitude (°) | 3.3100Ref | Proper motion in δ (mas/yr) | -5.67±0.01Ref |
Allen (1974) classified the object as a compact PN resembling a late-type star (his class S). He also claimed that most of the objects in this class are symbiotics or VV Cep-type stars. Nowadays, it is identified as a nebula with a WR central star, as reported for example by Esteban et al. (1991), Jiménez-Hernández et al. (2020), and Sévigny et al. (2021).