LIKELY
MILKY WAY
|
| GaSS 1-4 | IRAS - | GSC2.4.2 S5AY017432 | AAVSO - |
| SIMBAD UCAC4 290-063256 | Pan-STARRS - | SAO - | VSX 785968 |
| GAIA DR3 5403474822973970816 | SkyMapper 111215.48-320719.2 | WRAY - | GCVS - |
| 2MASS J11121548-3207193 | HIP - | Hen - | BD - |
| WISE J111215.47-320719.2 | 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 (°) | 168.0645Ref | Parallax (mas) | 0.123±0.017Ref | Reddening E(B-V) (mag) | 0.1±0.0Ref, Note |
| Declination (°) | -32.1220Ref | Distance (kpc) | 8.2Ref 7.23Ref, Note, 7.41Ref, Note |
||
| Galactic longitude (°) | 279.6093Ref | Proper motion in α (mas/yr) | 1.01±0.01Ref | ||
| Galactic latitude (°) | 26.2191Ref | Proper motion in δ (mas/yr) | -1.95±0.01Ref |
| X-Ray | NoRef | IR type | S?Ref | Radio | - |
| X-Ray type | - | J (mag) | 9.58Ref | Flickering | NoRef |
| GALEX FUV (mag) | - | H (mag) | 8.67Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 8.48Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 8.37Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 8.43Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 8.30Ref | IPmax (eV) | 13.6Ref |
| B (mag) | 14.42Ref | WISE W4 (mag) | 7.99Ref | [O III] lines | NoRef |
| V (mag) | 12.64Ref | IRAS 12μm (Jy) | - | He II lines | NoRef |
| R (mag) | 12.17Ref | IRAS 25μm (Jy) | - | [Fe VII] lines | NoRef |
| I (mag) | - | IRAS 60μm (Jy) | - | O VI lines | NoRef |
| BP (mag) | 12.89Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 11.91Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 10.93Ref | AKARI S18 (Jy) | - |
| Orbital period (days) | 458.92±4.25Ref | γ velocity (km/h) | 143.37±1.25Ref | Size of giant’s orbit (AU) | - |
| Eccentricity | 0.06±0.04Ref | RV of giant (km/h) | - | Separation (AU) | - |
| Inclination (°) | - | Inferior conj. of giant (JD) | - | Mass function | - |
| Eclipses | - | Mass ratio | - | ||
| Orbital ephemeris | Min (V) = 2457065 + 235 x ERef |
| Spectral type | M1Ref | Mass (M⊙) | - | Pulsation | - |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | - |
| IR type | S?Ref | Luminosity (L⊙) | - | Pulsation period (days) | - |
| Metallicity [Fe/H] | - | Pulsation ephemeris | - |
| Type/Spectral type | - | Mass (M⊙) | - | Spin period (min) | - |
| Shell-burning/Accreting-only | accreting-only?Ref | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | - |
This candidate for the accreting-only symbiotic star was identified in the GALAH high-resolution spectroscopic survey (Munari et al., 2021). A reported orbital period of 459 days from Gaia data (Beck et al. (2023)), double in comparison with the period observed in photometry by Munari et al., 2021, suggests that the giant might be close to filling its Roche-lobe.