SUSPECTED
LMC
|
| [RP2006] 883 | IRAS - | GSC2.4.2 S1HE049881 | AAVSO - |
| SIMBAD [RP2006] 883 | Pan-STARRS - | SAO - | VSX 2219018 |
| GAIA DR3 4657696495585686016 | SkyMapper 053556.90-690045.1 | WRAY - | GCVS - |
| 2MASS J05355689-6900450 | HIP - | Hen - | BD - |
| WISE J053556.87-690046.1 | TYC - | ESO - | HD - |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | [RP2006] 883 (Susp.) |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
| Right ascension (°) | 83.9871Ref | Parallax (mas) | -0.085±0.073Ref | Reddening E(B-V) (mag) | 1.9±0.46Ref, Note |
| Declination (°) | -69.0125Ref | Distance (kpc) | 49.97±0.19Ref 12.42Ref, Note, 10.20Ref, Note |
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| Galactic longitude (°) | 279.3964Ref | Proper motion in α (mas/yr) | 1.57±0.10Ref | ||
| Galactic latitude (°) | -31.9271Ref | Proper motion in δ (mas/yr) | 0.76±0.09Ref |
| X-Ray | NoRef | IR type | D'?Ref | Radio | - |
| X-Ray type | - | J (mag) | 13.12Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 12.15Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 12.63Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 9.84Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 8.91Ref | Resolved nebula | - |
| U (mag) | 18.43Ref | WISE W3 (mag) | 6.60Ref | IPmax (eV) | - |
| B (mag) | 18.75Ref | WISE W4 (mag) | 5.03Ref | [O III] lines | - |
| V (mag) | 18.23Ref | IRAS 12μm (Jy) | - | He II lines | - |
| R (mag) | 17.21Ref | IRAS 25μm (Jy) | - | [Fe VII] lines | - |
| I (mag) | 16.90Ref | IRAS 60μm (Jy) | - | O VI lines | - |
| BP (mag) | 18.01Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 17.54Ref | AKARI S09 (Jy) | 0.08Ref | ||
| RP (mag) | 16.77Ref | AKARI S18 (Jy) | - |
| Orbital period (days) | 176.49Ref | 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) | - | 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) | - |
[RP2006] 883 exhibits a strong nebular component in the optical, coupled with NIR and MIR colors indicative of an obscured RGB or AGB star, as observed in Miszalski et al. (2011). Additionally, Reid (2014) reported the presence of a dense, compact nebula and a weak continuum, suggesting characteristics of a weakly interacting symbiotic system.