SUSPECTED
MILKY WAY
|
| Gaia DR3 4110870983327739008 | IRAS - | GSC2.4.2 S8D5032733 | AAVSO 000-BMP-164 |
| SIMBAD [KW2003] 11 | Pan-STARRS 78762611664844483 | SAO - | VSX 608210 |
| GAIA DR3 4110870983327739008 | SkyMapper 172439.95-242147.4 | WRAY - | GCVS V3664 Oph |
| 2MASS J17243996-2421474 | HIP - | Hen - | BD - |
| WISE J172439.95-242147.5 | 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 (°) | 261.1665Ref | Parallax (mas) | 0.142±0.046Ref | Reddening E(B-V) (mag) | 0.7±0.02Ref, Note |
| Declination (°) | -24.3632Ref | Distance (kpc) | 5.31Ref, Note, 5.33Ref, Note | ||
| Galactic longitude (°) | 1.3346Ref | Proper motion in α (mas/yr) | -4.55±0.05Ref | ||
| Galactic latitude (°) | 6.4059Ref | Proper motion in δ (mas/yr) | -8.30±0.03Ref |
| X-Ray | - | IR type | - | Radio | - |
| X-Ray type | - | J (mag) | 9.20Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 7.95Ref | Outbursts | YesRef |
| GALEX NUV (mag) | - | K (mag) | 7.42Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 7.12Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 7.25Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 6.71Ref | IPmax (eV) | 35.1Ref |
| B (mag) | 17.24Ref | WISE W4 (mag) | 6.44Ref | [O III] lines | YesRef |
| V (mag) | - | IRAS 12μm (Jy) | - | He II lines | NoRef |
| R (mag) | 16.11Ref | IRAS 25μm (Jy) | - | [Fe VII] lines | NoRef |
| I (mag) | - | IRAS 60μm (Jy) | - | O VI lines | NoRef |
| BP (mag) | 15.99Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 14.02Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 12.49Ref | 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 | M?Ref | Mass (M⊙) | - | Pulsation | - |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | - |
| IR type | - | 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) | - |
Classified as a symbiotic star by Rimoldini et al. (2023) based on a machine-learning technique applied to Gaia DR3 data, including astrometric, photometric, and photometric time series information. Additionally, it has been classified as a Mira variable by Heinze et al. (2018) and as a classical nova by Aydi et al. (2018). It is mentioned as a symbiotic nova by Zuckerman et al. (2023).