MISCLASSIFIED
MILKY WAY
|
PN Hb 7 | IRAS 18523-3219 | GSC2.4.2 S9UU225333 | AAVSO - |
SIMBAD PN Hb 7 | Pan-STARRS 69282839074824058 | SAO - | VSX - |
GAIA DR3 6759935304494857984 | SkyMapper 185537.80-321548.6 | WRAY 16-422 | GCVS - |
2MASS J18553780-3215485 | HIP - | Hen 2-425 | BD - |
WISE J185537.83-321548.5 | TYC - | ESO 458-9 | HD 175194 |
Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
Right ascension (°) | 283.9075Ref | Parallax (mas) | 0.198±0.057Ref | Reddening E(B-V) (mag) | 0.12±0.0Ref, Note |
Declination (°) | -32.2635Ref | Distance (kpc) | 4.28Ref, Note, 4.41Ref, Note | ||
Galactic longitude (°) | 3.9636Ref | Proper motion in α (mas/yr) | -4.01±0.06Ref | ||
Galactic latitude (°) | -14.9025Ref | Proper motion in δ (mas/yr) | -6.90±0.05Ref |
In Allen & Glass (1974), it was suggested, based on infrared photometry, that this southern PN shows a continuum similar to symbiotic and VV Cephei stars. It was listed as a true PN in Acker et al. (1992).