MISCLASSIFIED
MILKY WAY
|
K 1-6 | IRAS - | GSC2.4.2 N0V3000606 | AAVSO 000-BNP-839 |
SIMBAD PN K 1-6 | Pan-STARRS 197313010594582765 | SAO - | VSX 168811 |
GAIA DR3 2288467186442571008 | SkyMapper - | WRAY - | GCVS V0434 Dra |
2MASS J20041428+7425364 | HIP - | Hen - | BD - |
WISE J200414.29+742536.0 | TYC 4458-557-1 | 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 (°) | 301.0595Ref | Parallax (mas) | 3.864±0.030Ref | Reddening E(B-V) (mag) | 0.18±0.01Ref, Note |
Declination (°) | 74.4266Ref | Distance (kpc) | 0.26Ref, Note, 0.26Ref, Note | ||
Galactic longitude (°) | 107.0357Ref | Proper motion in α (mas/yr) | -0.20±0.04Ref | ||
Galactic latitude (°) | 21.3839Ref | Proper motion in δ (mas/yr) | -28.19±0.05Ref |
Identified as an asymmetric planetary nebula with a binary central star (Frew et al., 2013), the symbiotic classification is deemed improbable according to their findings. Exhibiting variability with a period of 21 days, this object has been detected in X-rays, UV, and IR. The dynamic age is estimated at 19,500 years, with a distance of 760 pc as inferred by Ali et al. (2012). Further confirming its non-symbiotic nature, Merc et al. (2021) conducted a spectral analysis of the object.