MISCLASSIFIED
MILKY WAY
|
PN H1-43 | IRAS 17549-3347 | GSC2.4.2 S8GW040360 | AAVSO - |
SIMBAD PN H 1-43 | Pan-STARRS - | SAO - | VSX - |
GAIA DR3 4042380857826322176 | SkyMapper - | WRAY 16-335 | GCVS - |
2MASS J17581444-3347375 | HIP - | Hen 2-313 | BD - |
WISE - | TYC - | ESO 394-15 | HD - |
Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
Right ascension (°) | 269.5602Ref | Parallax (mas) | 0.571±0.061Ref | Reddening E(B-V) (mag) | 0.57±0.04Ref, Note |
Declination (°) | -33.7938Ref | Distance (kpc) | 1.66Ref, Note, 1.70Ref, Note | ||
Galactic longitude (°) | 357.1835Ref | Proper motion in α (mas/yr) | -1.39±0.07Ref | ||
Galactic latitude (°) | -4.7886Ref | Proper motion in δ (mas/yr) | -5.90±0.04Ref |
In 1974, based on infrared photometry, it was suggested by Allen & Glass (1974) that this southern planetary nebula exhibits a continuum similar to that of symbiotic and VV Cephei stars. In Acker et al. (1992), the target is classified as a true PN.