MISCLASSIFIED
LMC
|
[RP2006] 698 | IRAS 05339-6954 | GSC2.4.2 S0U9254871 | AAVSO - |
SIMBAD [RP2006] 698 | Pan-STARRS - | SAO - | VSX - |
GAIA DR3 4657999647407740672 | SkyMapper 053330.51-695226.9 | WRAY - | GCVS - |
2MASS J05333052-6952270 | HIP - | Hen - | BD - |
WISE J053330.56-695227.1 | 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 (°) | 83.3771Ref | Parallax (mas) | 1.132±0.286Ref | Reddening E(B-V) (mag) | 0.98±0.23Ref, Note |
Declination (°) | -69.8742Ref | Distance (kpc) | 49.97±0.19Ref 1.03Ref, Note, 1.89Ref, Note |
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Galactic longitude (°) | 280.4368Ref | Proper motion in α (mas/yr) | 3.54±0.35Ref | ||
Galactic latitude (°) | -32.0239Ref | Proper motion in δ (mas/yr) | -1.22±0.37Ref |
The classification of this star has varied over time. Initially, in Reid & Parker (2006), it was considered a possible symbiotic star. However, subsequent classifications in Reid & Parker (2012) labeled it as a B giant. Another classification in Miszalski et al. (2011) identified the object as an HII region, suggesting a dusty environment based on VMC and SAGE data. The most recent classification in Reid (2014) categorized it as an emission line star.