CONFIRMED
MILKY WAY
|
| Gaia DR2 6043925532812301184 | IRAS - | GSC2.4.2 S8QZ056413 | AAVSO 000-BNG-636 |
| SIMBAD Haro 1-10 | Pan-STARRS 72862469573175115 | SAO - | VSX 894777 |
| GAIA DR3 6043925532812301184 | SkyMapper 162749.75-291645.4 | WRAY 15-1491 | GCVS - |
| 2MASS J16274976-2916453 | HIP - | Hen - | BD - |
| WISE J162749.75-291645.4 | 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 (°) | 246.9573Ref | Parallax (mas) | 0.040±0.026Ref | Reddening E(B-V) (mag) | 0.33±0.02Ref, Note |
| Declination (°) | -29.2793Ref | Distance (kpc) | 9.11Ref, Note, 7.78Ref, Note | ||
| Galactic longitude (°) | 349.5167Ref | Proper motion in α (mas/yr) | -3.98±0.03Ref | ||
| Galactic latitude (°) | 13.4273Ref | Proper motion in δ (mas/yr) | -5.07±0.02Ref |
| X-Ray | YesRef | IR type | SRef | Radio | - |
| X-Ray type | δRef | J (mag) | 9.59Ref | Flickering | YesRef |
| GALEX FUV (mag) | - | H (mag) | 8.61Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 8.26Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 8.11Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 8.17Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 7.84Ref | IPmax (eV) | 35.1Ref |
| B (mag) | 15.75Ref | WISE W4 (mag) | 7.76Ref | [O III] lines | YesRef |
| V (mag) | 14.20Ref | IRAS 12μm (Jy) | - | He II lines | NoRef |
| R (mag) | 14.11Ref | IRAS 25μm (Jy) | - | [Fe VII] lines | NoRef |
| I (mag) | - | IRAS 60μm (Jy) | - | O VI lines | NoRef |
| BP (mag) | 14.78Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 13.11Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 11.83Ref | AKARI S18 (Jy) | - |
| Orbital period (days) | - | γ velocity (km/h) | -94.24±1.46Ref | 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 | M6 IIIRef | Mass (M⊙) | - | Pulsation | - |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | - |
| IR type | SRef | Luminosity (L⊙) | - | Pulsation period (days) | - |
| 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) | - |
Selected as a symbiotic candidate for an AAVSO observing campaign (Waagen, 2020) by Adrian B. Lucy from Columbia University. This object is identified as a long-period variable in Gaia DR2 (Mowlavi et al., 2018). The symbiotic nature of this system was subsequently confirmed in a detailed study by Lucy (2021).