MISCLASSIFIED
MILKY WAY
|
Hen 2-440 | IRAS 19360+2508 | GSC2.4.2 N22R142432 | AAVSO - |
SIMBAD Hen 2-440 | Pan-STARRS 138312945348414194 | SAO - | VSX - |
GAIA DR3 2021459171418312832 | SkyMapper - | WRAY - | GCVS - |
2MASS J19380836+2515409 | HIP - | Hen 2-440 | BD - |
WISE - | 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 (°) | 294.5348Ref | Parallax (mas) | 0.074±0.141Ref | Reddening E(B-V) (mag) | 1.77±0.09Ref, Note |
Declination (°) | 25.2613Ref | Distance (kpc) | 9.02Ref, Note, 3.83Ref, Note | ||
Galactic longitude (°) | 60.5441Ref | Proper motion in α (mas/yr) | -2.69±0.10Ref | ||
Galactic latitude (°) | 1.8172Ref | Proper motion in δ (mas/yr) | -6.03±0.15Ref |
Initially classified by Allen (1974) as a compact PN resembling a late-type star (his class S), with the assertion that most objects in this class are symbiotics or VV Cep-type stars. Later classifications, such as Acker et al. (1992) and García-Hernández & Górny (2014), suggested a true PN nature.