CONFIRMED
MILKY WAY
|
| Gaia DR2 5917238398632196736 | IRAS - | GSC2.4.2 S7HU008283 | AAVSO 000-BNG-639 |
| SIMBAD Gaia DR3 5917238398632196736 | Pan-STARRS - | SAO - | VSX 894780 |
| GAIA DR3 5917238398632196736 | SkyMapper 170710.55-565317.5 | WRAY - | GCVS - |
| 2MASS J17071056-5653174 | HIP - | Hen - | BD - |
| WISE J170710.55-565317.4 | 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 (°) | 256.7940Ref | Parallax (mas) | 0.027±0.032Ref | Reddening E(B-V) (mag) | 0.14±0.01Ref, Note |
| Declination (°) | -56.8882Ref | Distance (kpc) | 11.55Ref, Note, 8.19Ref, Note | ||
| Galactic longitude (°) | 332.7875Ref | Proper motion in α (mas/yr) | -3.43±0.02Ref | ||
| Galactic latitude (°) | -9.6895Ref | Proper motion in δ (mas/yr) | -2.20±0.02Ref |
| X-Ray | - | IR type | SRef | Radio | - |
| X-Ray type | - | J (mag) | 9.18Ref | Flickering | YesRef |
| GALEX FUV (mag) | - | H (mag) | 8.24Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 7.93Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 7.86Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 7.94Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 7.68Ref | IPmax (eV) | 13.6Ref |
| B (mag) | - | WISE W4 (mag) | 7.52Ref | [O III] lines | NoRef |
| V (mag) | 14.30Ref | 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) | 14.73Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 12.70Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 11.37Ref | AKARI S18 (Jy) | - |
| Orbital period (days) | - | γ velocity (km/h) | -90.65±1.31Ref | 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 | M5 IIIRef | Mass (M⊙) | - | Pulsation | - |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | - |
| IR type | SRef | Luminosity (L⊙) | - | Pulsation period (days) | - |
| Metallicity [Fe/H] | - | Pulsation ephemeris | - |
| Type/Spectral type | - | 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) | - |
Selected as a symbiotic candidate for the AAVSO observing campaign (AAVSO Alert Notice 681) by Adrian B. Lucy from Columbia University, the target was subsequently confirmed as a symbiotic star by Lucy (2021).