SUSPECTED
MILKY WAY
|
| IRAS 08034-0641 | IRAS 08034-0641 | GSC2.4.2 S3QU075322 | AAVSO - |
| SIMBAD IRAS 08034-0641 | Pan-STARRS 99781214732139319 | SAO - | VSX 411029 |
| GAIA DR3 3063985074325346432 | SkyMapper 080553.56-065033.2 | WRAY - | GCVS - |
| 2MASS J08055356-0650332 | HIP - | Hen - | BD - |
| WISE J080553.57-065033.3 | 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 (°) | 121.4732Ref | Parallax (mas) | 0.326±0.058Ref | Reddening E(B-V) (mag) | 0.06±0.0Ref, Note |
| Declination (°) | -6.8426Ref | Distance (kpc) | 2.72Ref, Note, 2.62Ref, Note | ||
| Galactic longitude (°) | 227.8429Ref | Proper motion in α (mas/yr) | -2.43±0.06Ref | ||
| Galactic latitude (°) | 13.1631Ref | Proper motion in δ (mas/yr) | -0.01±0.04Ref |
| X-Ray | - | IR type | - | Radio | - |
| X-Ray type | - | J (mag) | 6.62Ref | Flickering | - |
| GALEX FUV (mag) | 21.06Ref | H (mag) | 5.58Ref | Outbursts | - |
| GALEX NUV (mag) | 21.62Ref | K (mag) | 5.25Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 5.13Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 5.04Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 4.78Ref | IPmax (eV) | - |
| B (mag) | 14.02Ref | WISE W4 (mag) | 4.37Ref | [O III] lines | - |
| V (mag) | 12.45Ref | IRAS 12μm (Jy) | 0.41Ref | He II lines | - |
| R (mag) | - | IRAS 25μm (Jy) | 0.25Ref | [Fe VII] lines | - |
| I (mag) | - | IRAS 60μm (Jy) | 0.40Ref | O VI lines | - |
| BP (mag) | 12.81Ref | IRAS 100μm (Jy) | 1.20Ref | ||
| G (mag) | 10.39Ref | AKARI S09 (Jy) | 0.59Ref | ||
| RP (mag) | 9.00Ref | 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 | - | 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.