MISCLASSIFIED
MILKY WAY
|
Gaia 17bms | IRAS - | GSC2.4.2 N1AM098447 | AAVSO 000-BMH-961 |
SIMBAD - | Pan-STARRS 174573220837906634 | SAO - | VSX 479006 |
GAIA DR3 2177784092519048704 | SkyMapper - | WRAY - | GCVS - |
2MASS J21282005+5528479 | HIP - | Hen - | 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 (°) | 322.0838Ref | Parallax (mas) | 1.441±0.130Ref | Reddening E(B-V) (mag) | 1.78±0.1Ref, Note |
Declination (°) | 55.4799Ref | Distance (kpc) | 0.71Ref, Note, 0.72Ref, Note | ||
Galactic longitude (°) | 96.8463Ref | Proper motion in α (mas/yr) | 15.86±0.15Ref | ||
Galactic latitude (°) | 3.2542Ref | Proper motion in δ (mas/yr) | -4.55±0.17Ref |
Considered a candidate symbiotic star based on photometric appearance (Corradi et al., 2008), it is also listed as a confirmed symbiotic star in the ASAS-SN database (Jayasinghe et al., 2019). It has been detected in brightening by Gaia and the system was classified as an eclipsing CV with an orbital period of 0.145 days (Inight & Copperwheat, 2019).