CONFIRMED
LMC
|
| LMC S154 | IRAS F04533-7508 | GSC2.4.2 S0VX000383 | AAVSO 000-BCZ-119 |
| SIMBAD LHA 120-S 154 | Pan-STARRS - | SAO - | VSX 54635 |
| GAIA DR3 4649246748682812032 | SkyMapper 045150.45-750335.3 | WRAY - | GCVS - |
| 2MASS J04515046-7503353 | HIP - | Hen - | BD - |
| WISE J045150.46-750335.2 | TYC - | ESO - | HD - |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | LMC S154 (Conf.) |
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | LMC S154 (Conf.) |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
| Right ascension (°) | 72.9603Ref | Parallax (mas) | 0.036±0.029Ref | Reddening E(B-V) (mag) | 0.11±0.01Ref, Note |
| Declination (°) | -75.0598Ref | Distance (kpc) | 49.97±0.19Ref 10.44Ref, Note, 10.76Ref, Note |
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| Galactic longitude (°) | 287.3472Ref | Proper motion in α (mas/yr) | 2.24±0.04Ref | ||
| Galactic latitude (°) | -33.7068Ref | Proper motion in δ (mas/yr) | -0.13±0.03Ref |
| X-Ray | YesRef | IR type | SRef | Radio | - |
| X-Ray type | - | J (mag) | 11.71Ref | Flickering | - |
| GALEX FUV (mag) | 16.12Ref | H (mag) | 10.36Ref | Outbursts | YesRef |
| GALEX NUV (mag) | 17.36Ref | K (mag) | 9.38Ref | Outburst type | SyRNRef |
| IUE | YesRef | WISE W1 (mag) | 8.64Ref | Jets | - |
| FUSE | YesRef | WISE W2 (mag) | 7.98Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 6.78Ref | IPmax (eV) | 290.9Ref |
| B (mag) | 12.80Ref | WISE W4 (mag) | 6.24Ref | [O III] lines | YesRef |
| V (mag) | 15.70Ref | IRAS 12μm (Jy) | 0.10Ref | He II lines | YesRef |
| R (mag) | 14.20Ref | IRAS 25μm (Jy) | 0.05Ref | [Fe VII] lines | YesRef |
| I (mag) | 13.20Ref | IRAS 60μm (Jy) | 0.07Ref | O VI lines | YesRef |
| BP (mag) | 16.10Ref | IRAS 100μm (Jy) | 0.78Ref | ||
| G (mag) | 15.48Ref | AKARI S09 (Jy) | 0.12Ref | ||
| RP (mag) | 14.56Ref | 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 | C2.2Ref | Mass (M⊙) | 2Ref | Pulsation | YesRef |
| Eff. temperature (K) | 4000±250Ref | Radius (R⊙) | 400Ref | Type | quasi-periodicRef |
| IR type | SRef | Luminosity (L⊙) | 12000Ref, 12300Ref | Pulsation period (days) | 250Ref |
| Metallicity [Fe/H] | - | Pulsation ephemeris | - |
| Type/Spectral type | - | Mass (M⊙) | - | Spin period (min) | - |
| Shell-burning/Accreting-only | shell-burningRef | Radius (R⊙) | 0.092Ref | Accretion disk | - |
| Eff. temperature (K) | 125000-155000Ref | Luminosity (L⊙) | 2000-4000Ref | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | - |
The star underwent a transformation in its spectral appearance, transitioning from a low-excitation emission line object to that of a symbiotic star, likely due to the optical thinning of the nebula (Remillard et al., 1992). Subsequent analysis of archival observations in Iłkiewicz et al. (2019) supports the classification of the object as a symbiotic recurrent nova.