POSSIBLE
MILKY WAY
|
| GaSS 1-24 | IRAS - | GSC2.4.2 S7G3000483 | AAVSO 000-BDG-714 |
| SIMBAD V* V818 Ara | Pan-STARRS - | SAO - | VSX 3621 |
| GAIA DR3 5913483635125475328 | SkyMapper 171744.37-613805.3 | WRAY - | GCVS V0818 Ara |
| 2MASS J17174438-6138052 | HIP - | Hen - | BD - |
| WISE J171744.37-613805.4 | 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 (°) | 259.4349Ref | Parallax (mas) | 0.090±0.023Ref | Reddening E(B-V) (mag) | 0.09±0.0Ref, Note |
| Declination (°) | -61.6348Ref | Distance (kpc) | 9.49Ref, Note, 6.65Ref, Note | ||
| Galactic longitude (°) | 329.5658Ref | Proper motion in α (mas/yr) | 0.03±0.02Ref | ||
| Galactic latitude (°) | -13.4824Ref | Proper motion in δ (mas/yr) | -6.80±0.02Ref |
| X-Ray | - | IR type | S?Ref | Radio | - |
| X-Ray type | - | J (mag) | 9.00Ref | Flickering | NoRef |
| GALEX FUV (mag) | - | H (mag) | 8.02Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 7.79Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 7.67Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 7.74Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 7.25Ref | IPmax (eV) | 13.6Ref |
| B (mag) | 14.89Ref | WISE W4 (mag) | 6.82Ref | [O III] lines | NoRef |
| V (mag) | 13.00Ref | 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) | 13.03Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 11.76Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 10.57Ref | AKARI S18 (Jy) | - |
| Orbital period (days) | - | γ velocity (km/h) | 174.15±0.49Ref | 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 | M6Ref | Mass (M⊙) | - | Pulsation | Yes?Ref |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | SRaRef |
| IR type | S?Ref | Luminosity (L⊙) | - | Pulsation period (days) | 364Ref |
| Metallicity [Fe/H] | - | Pulsation ephemeris | - |
| Type/Spectral type | - | Mass (M⊙) | - | Spin period (min) | - |
| Shell-burning/Accreting-only | accreting-only?Ref | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | - |
Candidate for the accreting-only symbiotic star selected from the GALAH high-resolution spectroscopic survey (Munari et al., 2021). This object is also classified as an SRa variable with a period of 364 days, according to VSX (Watson et al., 2006).