MISCLASSIFIED
MILKY WAY
|
KT Eri | IRAS - | GSC2.4.2 S2B7000318 | AAVSO 000-BJR-847 |
SIMBAD KT Eri | Pan-STARRS 95780719758286017 | SAO - | VSX 238721 |
GAIA DR3 3184664584368981760 | SkyMapper 044754.20-101043.1 | WRAY - | GCVS KT Eri |
2MASS J04475419-1010429 | HIP - | Hen - | BD - |
WISE J044754.20-101042.7 | 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 (°) | 71.9759Ref | Parallax (mas) | 0.196±0.025Ref | Reddening E(B-V) (mag) | 0.08±0.0Ref, Note |
Declination (°) | -10.1786Ref | Distance (kpc) | 4.06Ref, Note, 3.90Ref, Note | ||
Galactic longitude (°) | 207.9863Ref | Proper motion in α (mas/yr) | 6.47±0.02Ref | ||
Galactic latitude (°) | -32.0202Ref | Proper motion in δ (mas/yr) | -11.07±0.02Ref |
The nova outburst of KT Eri was discovered in 2009 (Itagaki, 2009). A possible analogy to symbiotic stars was suggested by Jurdana-Šepić et al. (2012), who detected a period of 737 days in its light curve. However, Munari & Dallaporta (2014) contradicted the symbiotic nature of the object, arguing that the star is too faint in the infrared to contain a Roche-lobe filling giant. They proposed an alternative classification of a CV in a triple system for KT Eri.