MISCLASSIFIED
MILKY WAY
|
SS73 22 | IRAS 10197-5750 | GSC2.4.2 S47O000556 | AAVSO - |
SIMBAD MR 22 | Pan-STARRS - | SAO - | VSX 431861 |
GAIA DR3 5255657029503679360 | SkyMapper 102133.84-580547.9 | WRAY 15-549 | GCVS - |
2MASS J10213385-5805476 | HIP - | Hen 3-404 | BD - |
WISE J102133.84-580547.4 | TYC - | ESO - | HD - |
Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | VDS 24 (Conf.) |
Right ascension (°) | 155.3910Ref | Parallax (mas) | - | Reddening E(B-V) (mag) | 3.12±0.91Ref, Note |
Declination (°) | -58.0962Ref | Distance (kpc) | -, Note |
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Galactic longitude (°) | 284.1766Ref | Proper motion in α (mas/yr) | - | ||
Galactic latitude (°) | -0.7899Ref | Proper motion in δ (mas/yr) | - |
Classified as a symbiotic star by Sanduleak & Stephenson (1973), who suspected He II emission in addition to Hα and Hβ lines. However, Allen et al. (1980) detected only Balmer lines in emission and suspected a pre-main-sequence object. The star is listed among confirmed symbiotic stars by Vaidis (1988). Additionally, it is included in the lists of both pre-planetary nebulae (Kohoutek, 2001) and planetary nebulae (Frew et al., 2013). The object is also classified as a likely post-AGB star (Vickers et al., 2015).