SUSPECTED
MILKY WAY
|
| AN Tel | IRAS - | GSC2.4.2 SAUO061144 | AAVSO 000-BFN-296 |
| SIMBAD V* AN Tel | Pan-STARRS - | SAO - | VSX 36310 |
| GAIA DR3 6650202742655689344 | SkyMapper 184639.05-552113.0 | WRAY - | GCVS AN Tel |
| 2MASS J18463907-5521129 | HIP - | Hen - | BD - |
| WISE J184639.06-552113.1 | TYC 8762-33-1 | 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 (°) | 281.6627Ref | Parallax (mas) | 0.376±0.018Ref | Reddening E(B-V) (mag) | 0.07±0.0Ref, Note |
| Declination (°) | -55.3536Ref | Distance (kpc) | 2.48Ref, Note, 2.45Ref, Note | ||
| Galactic longitude (°) | 340.5506Ref | Proper motion in α (mas/yr) | -0.50±0.01Ref | ||
| Galactic latitude (°) | -21.3804Ref | Proper motion in δ (mas/yr) | -0.30±0.01Ref |
| X-Ray | - | IR type | - | Radio | - |
| X-Ray type | - | J (mag) | 7.94Ref | Flickering | - |
| GALEX FUV (mag) | 20.78Ref | H (mag) | 7.10Ref | Outbursts | - |
| GALEX NUV (mag) | 19.86Ref | K (mag) | 6.96Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 6.84Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 6.86Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 6.54Ref | IPmax (eV) | 0Ref |
| B (mag) | 12.48Ref | WISE W4 (mag) | 6.19Ref | [O III] lines | NoRef |
| V (mag) | 10.85Ref | IRAS 12μm (Jy) | - | He II lines | NoRef |
| R (mag) | - | IRAS 25μm (Jy) | - | [Fe VII] lines | NoRef |
| I (mag) | - | IRAS 60μm (Jy) | - | O VI lines | NoRef |
| BP (mag) | 11.13Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 10.20Ref | AKARI S09 (Jy) | 0.18Ref | ||
| RP (mag) | 9.24Ref | AKARI S18 (Jy) | - |
| Orbital period (days) | - | γ velocity (km/h) | 31.33±0.52Ref | 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 | accreting-onlyRef | 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. However, their spectroscopic observations did not reveal any emission lines, leading to the suggestion that this star is an accreting-only symbiotic candidate.