SUSPECTED
MILKY WAY
|
| BD-19 2567 | IRAS 08534-1954 | GSC2.4.2 S5VU000472 | AAVSO - |
| SIMBAD BD-19 2567 | Pan-STARRS 83871339228469389 | SAO - | VSX 88265 |
| GAIA DR3 5704427648170340224 | SkyMapper 085541.56-200603.1 | WRAY - | GCVS - |
| 2MASS J08554155-2006034 | HIP - | Hen - | BD -19 2567 |
| WISE J085541.55-200603.1 | TYC 6021-1288-1 | 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 (°) | 133.9231Ref | Parallax (mas) | 0.751±0.032Ref | Reddening E(B-V) (mag) | 0.15±0.01Ref, Note |
| Declination (°) | -20.1009Ref | Distance (kpc) | 1.27Ref, Note, 1.27Ref, Note | ||
| Galactic longitude (°) | 246.1530Ref | Proper motion in α (mas/yr) | -5.57±0.03Ref | ||
| Galactic latitude (°) | 15.9348Ref | Proper motion in δ (mas/yr) | 9.49±0.03Ref |
| X-Ray | - | IR type | - | Radio | - |
| X-Ray type | - | J (mag) | 4.73Ref | Flickering | - |
| GALEX FUV (mag) | 21.31Ref | H (mag) | 3.80Ref | Outbursts | - |
| GALEX NUV (mag) | 20.58Ref | K (mag) | 3.57Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 2.47Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 2.96Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 2.47Ref | IPmax (eV) | - |
| B (mag) | 11.78Ref | WISE W4 (mag) | 1.87Ref | [O III] lines | - |
| V (mag) | 9.97Ref | IRAS 12μm (Jy) | 4.49Ref | He II lines | - |
| R (mag) | - | IRAS 25μm (Jy) | 1.77Ref | [Fe VII] lines | - |
| I (mag) | - | IRAS 60μm (Jy) | 0.48Ref | O VI lines | - |
| BP (mag) | 10.20Ref | IRAS 100μm (Jy) | 1.29Ref | ||
| G (mag) | 8.10Ref | AKARI S09 (Jy) | 4.41Ref | ||
| RP (mag) | 6.77Ref | AKARI S18 (Jy) | 1.91Ref |
| Orbital period (days) | - | γ velocity (km/h) | 4.47±0.28Ref | 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 | - | Luminosity (L⊙) | - | Pulsation period (days) | - |
| 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.