SUSPECTED
SCULPTOR DWARF
|
| [SS2022] 58 | IRAS - | GSC2.4.2 S09V002679 | AAVSO - |
| SIMBAD 2MASS J01000005-3345287 | Pan-STARRS 67490150002310669 | SAO - | VSX - |
| GAIA DR3 5003198920551987456 | SkyMapper 005959.99-334528.9 | WRAY - | GCVS - |
| 2MASS J01000005-3345287 | HIP - | Hen - | BD - |
| WISE J010000.06-334528.7 | 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 (°) | 15.0002Ref | Parallax (mas) | 0.306±0.136Ref | Reddening E(B-V) (mag) | 0.02±0.0Ref, Note |
| Declination (°) | -33.7580Ref | Distance (kpc) | 2.49Ref, Note, 2.23Ref, Note | ||
| Galactic longitude (°) | 287.9091Ref | Proper motion in α (mas/yr) | -0.01±0.11Ref | ||
| Galactic latitude (°) | -83.1187Ref | Proper motion in δ (mas/yr) | -0.11±0.08Ref |
| X-Ray | YesRef | IR type | - | Radio | - |
| X-Ray type | - | J (mag) | 16.74Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 15.77Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 15.35Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 15.92Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 15.68Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 12.10Ref | IPmax (eV) | - |
| B (mag) | 19.28Ref | WISE W4 (mag) | 8.94Ref | [O III] lines | - |
| V (mag) | 18.33Ref | IRAS 12μm (Jy) | - | He II lines | - |
| R (mag) | - | IRAS 25μm (Jy) | - | [Fe VII] lines | - |
| I (mag) | 17.28Ref | IRAS 60μm (Jy) | - | O VI lines | - |
| BP (mag) | 18.66Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 18.12Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 17.43Ref | AKARI S18 (Jy) | - |
| Orbital period (days) | - | γ velocity (km/h) | - | Size of giant’s orbit (AU) | - |
| Eccentricity | - | RV of giant (km/h) | - | Separation (AU) | - |
| Inclination (°) | - | Inferior conj. of giant (JD) | - | Mass function | - |
| Eclipses | - | Mass ratio | - | ||
| Orbital ephemeris | - |
| Spectral type | - | Mass (M⊙) | - | Pulsation | - |
| Eff. temperature (K) | 4672±64Ref | Radius (R⊙) | - | Type | - |
| IR type | - | Luminosity (L⊙) | - | Pulsation period (days) | - |
| Metallicity [Fe/H] | -2.67Ref | Pulsation ephemeris | - |
| Type/Spectral type | - | Mass (M⊙) | - | Spin period (min) | - |
| Shell-burning/Accreting-only | - | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | - |
The star is suggested as a symbiotic candidate based on the detected X-ray emission and optical/IR counterpart, according to Saeedi & Sasaki (2022). RGB classification was reported in Chiti et al. (2018). It was incorrectly classified as an RR Lyr-type variable in SIMBAD (Wenger et al., 2000), with reference to the aforementioned paper.