SUSPECTED
LMC
|
| [RP2006] 803 | IRAS - | GSC2.4.2 S1HP100899 | AAVSO - |
| SIMBAD 2MASS J05240989-6919479 | Pan-STARRS - | SAO - | VSX - |
| GAIA DR3 4658086306860163584 | SkyMapper 052409.90-691948.0 | WRAY - | GCVS - |
| 2MASS J05240989-6919479 | HIP - | Hen - | BD - |
| WISE J052409.90-691947.8 | TYC - | ESO - | HD - |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | LMC SySt-15 (Susp.) |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
| Right ascension (°) | 81.0413Ref | Parallax (mas) | -0.057±0.049Ref | Reddening E(B-V) (mag) | 0.95±0.21Ref, Note |
| Declination (°) | -69.3300Ref | Distance (kpc) | 49.97±0.19Ref 9.93Ref, Note, 16.59Ref, Note |
||
| Galactic longitude (°) | 279.9550Ref | Proper motion in α (mas/yr) | 1.76±0.06Ref | ||
| Galactic latitude (°) | -32.9147Ref | Proper motion in δ (mas/yr) | 0.30±0.06Ref |
| X-Ray | NoRef | IR type | D'Ref | Radio | - |
| X-Ray type | - | J (mag) | 12.63Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 11.59Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 11.18Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 10.93Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 10.97Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 9.62Ref | IPmax (eV) | - |
| B (mag) | - | WISE W4 (mag) | 8.83Ref | [O III] lines | - |
| V (mag) | 18.81Ref | IRAS 12μm (Jy) | - | He II lines | - |
| R (mag) | 14.93Ref | IRAS 25μm (Jy) | - | [Fe VII] lines | - |
| I (mag) | 14.90Ref | IRAS 60μm (Jy) | - | O VI lines | - |
| BP (mag) | 18.77Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 16.55Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 15.12Ref | 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 | M3 IIIRef | Mass (M⊙) | - | Pulsation | - |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | - |
| IR type | D'Ref | Luminosity (L⊙) | - | Pulsation period (days) | - |
| Metallicity [Fe/H] | - | 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 very strong MIR colors, combined with a late-type M3III continuum and the presence of forbidden lines, suggest a symbiotic or possibly an interacting LTS (Reid, 2014).