SUSPECTED
MILKY WAY
|
| 2MASS J105143.65-270433.1 | IRAS - | GSC2.4.2 S59T000006 | AAVSO - |
| SIMBAD ATO J162.9316-27.0757 | Pan-STARRS 75501629316749385 | SAO - | VSX 92335 |
| GAIA DR3 5457817669781395456 | SkyMapper 105143.61-270432.7 | WRAY - | GCVS - |
| 2MASS J10514358-2704327 | HIP - | Hen - | BD - |
| WISE J105143.59-270432.7 | 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 (°) | 162.9317Ref | Parallax (mas) | 0.159±0.030Ref | Reddening E(B-V) (mag) | 0.07±0.0Ref, Note |
| Declination (°) | -27.0758Ref | Distance (kpc) | 5.69Ref, Note, 4.95Ref, Note | ||
| Galactic longitude (°) | 272.5252Ref | Proper motion in α (mas/yr) | -2.61±0.03Ref | ||
| Galactic latitude (°) | 28.6352Ref | Proper motion in δ (mas/yr) | 1.03±0.03Ref |
| X-Ray | - | IR type | - | Radio | - |
| X-Ray type | - | J (mag) | 9.00Ref | Flickering | - |
| GALEX FUV (mag) | 21.59Ref | H (mag) | 8.11Ref | Outbursts | - |
| GALEX NUV (mag) | 22.76Ref | K (mag) | 7.86Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 7.68Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 7.84Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 7.59Ref | IPmax (eV) | - |
| B (mag) | 14.15Ref | WISE W4 (mag) | 7.34Ref | [O III] lines | - |
| V (mag) | 12.46Ref | IRAS 12μm (Jy) | - | He II lines | - |
| R (mag) | 11.91Ref | IRAS 25μm (Jy) | - | [Fe VII] lines | - |
| I (mag) | - | IRAS 60μm (Jy) | - | O VI lines | - |
| BP (mag) | 12.74Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 11.58Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 10.51Ref | AKARI S18 (Jy) | - |
| Orbital period (days) | - | γ velocity (km/h) | 25.03±0.32Ref | 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 | Yes?Ref |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | SR?Ref |
| IR type | - | Luminosity (L⊙) | - | Pulsation period (days) | 334.2777619Ref |
| Metallicity [Fe/H] | - | Pulsation ephemeris | - |
| Type/Spectral type | WDRef | Mass (M⊙) | - | Spin period (min) | - |
| Shell-burning/Accreting-only | - | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | - |
Suspected of having a symbiotic nature by Akras (2023). The authors employed a combination of GALEX UV photometry, 2MASS/WISE IR photometry, and the ASAS-SN variables catalog to select the candidates.