January 13, 2024
New objects added
January 17, 2023
Gaia DR3 candidates added
January 15, 2023
Utilities and search added
January 4, 2023
New version fully released
November 7, 2022
New version testing started
Jan 28, 2019
First public release
All symbiotics
Galactic symbiotics
Extragalactic symbiotics
Version from February 3, 2024
SUSPECTED
MILKY WAY
|
| VPHASDR2J173155.9-301915.6 | IRAS - | GSC2.4.2 S8H0002689 | AAVSO - |
| SIMBAD 2MASS J17315586-3019155 | Pan-STARRS 71612629828105082 | SAO - | VSX - |
| GAIA DR3 4058438189969404032 | SkyMapper 173155.87-301915.6 | WRAY - | GCVS - |
| 2MASS J17315586-3019155 | HIP - | Hen - | BD - |
| WISE J173155.86-301915.6 | 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 (°) | 262.9828Ref | Parallax (mas) | 0.083±0.092Ref | Reddening E(B-V) (mag) | 2.33±0.15Ref, Note |
| Declination (°) | -30.3210Ref | Distance (kpc) | 7.20Ref, Note, 6.98Ref, Note | ||
| Galactic longitude (°) | 357.2410Ref | Proper motion in α (mas/yr) | 0.59±0.09Ref | ||
| Galactic latitude (°) | 1.7765Ref | Proper motion in δ (mas/yr) | -5.78±0.07Ref |
| X-Ray | NoRef | IR type | S?Ref | Radio | - |
| X-Ray type | - | J (mag) | 10.24Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 8.87Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 8.23Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 7.85Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 7.92Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 7.41Ref | IPmax (eV) | - |
| B (mag) | - | WISE W4 (mag) | 6.63Ref | [O III] lines | - |
| V (mag) | - | IRAS 12μm (Jy) | - | He II lines | - |
| R (mag) | - | IRAS 25μm (Jy) | - | [Fe VII] lines | - |
| I (mag) | - | IRAS 60μm (Jy) | - | O VI lines | - |
| BP (mag) | 18.08Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 15.60Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 14.09Ref | 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 | S?Ref | 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 possible symbiotic star based on infrared data by Akras et al. (2019), this object is also designated as a long-period variable by Mowlavi et al. (2018).