CONFIRMED
MILKY WAY
|
| THA 23-30 | IRAS - | GSC2.4.2 S8IH151443 | AAVSO - |
| SIMBAD THA 23-30 | Pan-STARRS 80292525117744529 | SAO - | VSX 571455 |
| GAIA DR3 4125688650452414848 | SkyMapper 165002.89-230517.7 | WRAY - | GCVS - |
| 2MASS J16500289-2305178 | HIP - | Hen - | BD - |
| WISE J165002.89-230517.7 | 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 (°) | 252.5120Ref | Parallax (mas) | 0.019±0.016Ref | Reddening E(B-V) (mag) | 0.43±0.02Ref, Note |
| Declination (°) | -23.0883Ref | Distance (kpc) | 11.15Ref, Note, 9.69Ref, Note | ||
| Galactic longitude (°) | 357.6870Ref | Proper motion in α (mas/yr) | -4.91±0.02Ref | ||
| Galactic latitude (°) | 13.5816Ref | Proper motion in δ (mas/yr) | -1.86±0.01Ref |
| X-Ray | - | IR type | SRef | Radio | - |
| X-Ray type | - | J (mag) | 9.89Ref | Flickering | - |
| GALEX FUV (mag) | 18.38Ref | H (mag) | 8.94Ref | Outbursts | - |
| GALEX NUV (mag) | 18.59Ref | K (mag) | 8.62Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 8.53Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 8.58Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 8.26Ref | IPmax (eV) | 114Ref |
| B (mag) | 16.20Ref | WISE W4 (mag) | 7.72Ref | [O III] lines | YesRef |
| V (mag) | 14.60Ref | IRAS 12μm (Jy) | - | He II lines | YesRef |
| R (mag) | 14.27Ref | IRAS 25μm (Jy) | - | [Fe VII] lines | NoRef |
| I (mag) | - | IRAS 60μm (Jy) | - | O VI lines | YesRef |
| BP (mag) | 14.82Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 13.17Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 11.93Ref | AKARI S18 (Jy) | - |
| Orbital period (days) | - | γ velocity (km/h) | -37.55±0.61Ref | 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 | M1Ref | Mass (M⊙) | - | Pulsation | Yes?Ref |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | SR?Ref |
| IR type | SRef | Luminosity (L⊙) | - | Pulsation period (days) | 334.37Ref |
| Metallicity [Fe/H] | - | Pulsation ephemeris | - |
| Type/Spectral type | WDRef | Mass (M⊙) | - | Spin period (min) | - |
| Shell-burning/Accreting-only | shell-burningRef | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | - |
Selected as a potential symbiotic star by Akras (2023), based on GALEX UV photometry, 2MASS/WISE IR photometry, and the ASAS-SN variables catalog. Their spectroscopic observations confirmed the symbiotic nature of this star. It was previously classified as an emission-line star by The & Lim (1964).