MISCLASSIFIED
MILKY WAY
|
5 Ceti | IRAS 00056-0243 | GSC2.4.2 S00C000063 | AAVSO 000-BBB-190 |
SIMBAD * 5 Cet | Pan-STARRS 105060020502663500 | SAO 28602 | VSX 26465 |
GAIA DR3 2448444655110889088 | SkyMapper 000812.09-022652.5 | WRAY - | GCVS AP Psc |
2MASS J00081208-0226518 | HIP 664 | Hen - | BD -03 3 |
WISE J000812.11-022651.8 | TYC 4663-363-1 | ESO - | HD 352 |
Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
Right ascension (°) | 2.0504Ref | Parallax (mas) | 2.768±0.068Ref | Reddening E(B-V) (mag) | 0.03±0.0Ref, Note |
Declination (°) | -2.4477Ref | Distance (kpc) | 0.36Ref, Note, 0.35Ref, Note | ||
Galactic longitude (°) | 98.3443Ref | Proper motion in α (mas/yr) | 6.58±0.08Ref | ||
Galactic latitude (°) | -63.2366Ref | Proper motion in δ (mas/yr) | -3.72±0.04Ref |
The potential symbiotic nature of this star is discussed by Eaton & Barden (1988). However, it is more likely a beta Lyrae system—a semi-detached binary with an orbital period of 96.4 days (Batten et al., 1978).