MISCLASSIFIED
MILKY WAY
|
PN M2-39 | IRAS 18189-2412 | GSC2.4.2 S9TG041811 | AAVSO - |
SIMBAD PN M 2-39 | Pan-STARRS 78982755047957056 | SAO - | VSX - |
GAIA DR3 4089299595925528832 | SkyMapper 182201.16-241039.8 | WRAY 15-1866 | GCVS - |
2MASS J18220114-2410398 | HIP - | Hen 2-391 | BD - |
WISE - | TYC - | ESO 522-20 | HD - |
Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
Right ascension (°) | 275.5048Ref | Parallax (mas) | 0.051±0.040Ref | Reddening E(B-V) (mag) | 0.53±0.01Ref, Note |
Declination (°) | -24.1778Ref | Distance (kpc) | 7.80Ref, Note, 5.97Ref, Note | ||
Galactic longitude (°) | 8.1477Ref | Proper motion in α (mas/yr) | -1.27±0.04Ref | ||
Galactic latitude (°) | -4.7508Ref | Proper motion in δ (mas/yr) | -3.57±0.03Ref |
In Allen (1974), the object was classified as a compact PN resembling a late-type star, falling into the class S according to the classification by the author. It was noted that most objects in this class are symbiotics or VV Cephei-type stars. Classified as a true PN in Acker et al. (1992).