MISCLASSIFIED
MILKY WAY
|
| XX Oph | IRAS 17412-0614 | GSC2.4.2 S7XN000022 | AAVSO 000-BBZ-287 |
| SIMBAD V* XX Oph | Pan-STARRS 100472659855947602 | SAO 141834 | VSX 20535 |
| GAIA DR3 4169184647552062464 | SkyMapper - | WRAY - | GCVS XX Oph |
| 2MASS J17435650-0616086 | HIP 86777 | Hen - | BD -06 4638 |
| WISE J174356.54-061609.0 | TYC 5093-346-1 | ESO - | HD 161114 |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
| Right ascension (°) | 265.9854Ref | Parallax (mas) | 0.467±0.101Ref | Reddening E(B-V) (mag) | 0.81±0.01Ref, Note |
| Declination (°) | -6.2691Ref | Distance (kpc) | 2.36Ref, Note, 2.18Ref, Note | ||
| Galactic longitude (°) | 19.4101Ref | Proper motion in α (mas/yr) | 1.31±0.10Ref | ||
| Galactic latitude (°) | 11.9465Ref | Proper motion in δ (mas/yr) | -6.28±0.07Ref |
Mentioned as a "symbiotic object featuring deep fadings of long duration" in GCVS with a reference to Shapley & Woods (1926), this star is also listed as a possible symbiotic star by Allen (1973). The star exhibits complex spectroscopic and photometric variations, as reported in Goswami et al. (2001). According to Goswami et al. (2001), the spectrum resembles that of the known symbiotic star MWC 560. On the other hand, Evans et al. (1993) claimed that the object is more likely a Zeta Aur/VV Cep system.