CONFIRMED
MILKY WAY
|
| 2SXPS J173508.4-292958 | IRAS - | GSC2.4.2 S8H0000151 | AAVSO 000-BNM-033 |
| SIMBAD UCAC4 303-143267 | Pan-STARRS 72602637846321003 | SAO - | VSX 1543884 |
| GAIA DR3 4058581921170339456 | SkyMapper 173508.31-292958.0 | WRAY - | GCVS - |
| 2MASS J17350831-2929580 | HIP - | Hen - | BD - |
| WISE J173508.32-292958.0 | 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 (°) | 263.7846Ref | Parallax (mas) | 0.669±0.020Ref | Reddening E(B-V) (mag) | 2.02±0.09Ref, Note |
| Declination (°) | -29.4995Ref | Distance (kpc) | 1.45Ref, Note, 1.43Ref, Note | ||
| Galactic longitude (°) | 358.3089Ref | Proper motion in α (mas/yr) | -0.78±0.03Ref | ||
| Galactic latitude (°) | 1.6395Ref | Proper motion in δ (mas/yr) | -2.42±0.02Ref |
| X-Ray | YesRef | IR type | SRef | Radio | - |
| X-Ray type | βRef | J (mag) | 8.51Ref | Flickering | NoRef |
| GALEX FUV (mag) | - | H (mag) | 7.76Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 7.44Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 7.05Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 7.28Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 7.26Ref | IPmax (eV) | - |
| B (mag) | 13.39Ref | WISE W4 (mag) | 7.34Ref | [O III] lines | - |
| V (mag) | 11.77Ref | IRAS 12μm (Jy) | - | He II lines | - |
| R (mag) | - | IRAS 25μm (Jy) | - | [Fe VII] lines | - |
| I (mag) | - | IRAS 60μm (Jy) | - | O VI lines | - |
| BP (mag) | 12.14Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 11.13Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 10.14Ref | AKARI S18 (Jy) | - |
| Orbital period (days) | - | γ velocity (km/h) | -12.00±1.00Ref | 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 | K4 IIIRef | Mass (M⊙) | - | Pulsation | YesRef |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | SRRef |
| IR type | SRef | Luminosity (L⊙) | - | Pulsation period (days) | 32.3Ref |
| 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) | - |
Confirmed as a symbiotic star of the accreting-only type, the classification is based on observations that include weak and structured emission in Hα, along with near-UV excess emission, as detailed in Munari et al. (2021).