MISCLASSIFIED
MILKY WAY
|
| V1017 Cyg | IRAS - | GSC2.4.2 N2HN048100 | AAVSO 000-BDN-956 |
| SIMBAD V* V1017 Cyg | Pan-STARRS 171982990659334762 | SAO - | VSX 11937 |
| GAIA DR3 2137557948519577472 | SkyMapper - | WRAY - | GCVS V1017 Cyg |
| 2MASS J19561580+5319119 | HIP - | Hen - | BD - |
| WISE J195615.81+531912.1 | 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 (°) | 299.0659Ref | Parallax (mas) | 0.817±0.021Ref | Reddening E(B-V) (mag) | 0.19±0.01Ref, Note |
| Declination (°) | 53.3200Ref | Distance (kpc) | 1.20Ref, Note, 1.18Ref, Note | ||
| Galactic longitude (°) | 86.9414Ref | Proper motion in α (mas/yr) | 6.18±0.03Ref | ||
| Galactic latitude (°) | 12.5514Ref | Proper motion in δ (mas/yr) | 5.42±0.03Ref |
Classified as a bona-fide symbiotic star in the study of post-AGB stars conducted by Szczerba et al. (2007). It is listed as a confirmed symbiotic star in SIMBAD (Wenger et al., 2000). Additionally, the star is also included in the catalogs of RR Lyr stars provided by Gavrilchenko et al. (2014) and Bramich et al. (2014). However, recent analysis by Merc et al. (2021), based on spectroscopic data and available photometry, proposed that the object is a W UMa variable, with a period of approximately 0.33 days.