CONFIRMED
NGC 6822
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| NGC 6822 SySt-1 | IRAS - | GSC2.4.2 SA0E055910 | AAVSO - |
| SIMBAD [SRC2012] 296.224487-14.863070 | Pan-STARRS 90162962244434685 | SAO - | VSX - |
| GAIA DR3 4182446338325490816 | SkyMapper - | WRAY - | GCVS - |
| 2MASS J19445377-1451463 | HIP - | Hen - | BD - |
| WISE J194453.82-145146.6 | TYC - | ESO - | HD - |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | NGC6822 SySt-1 (Conf.) |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
| Right ascension (°) | 296.2245Ref | Parallax (mas) | 0.060±0.841Ref | Reddening E(B-V) (mag) | 0.21±0.01Ref, Note |
| Declination (°) | -14.8631Ref | Distance (kpc) | 500±10Ref 5.12Ref, Note, 2.63Ref, Note |
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| Galactic longitude (°) | 25.2754Ref | Proper motion in α (mas/yr) | -1.48±0.99Ref | ||
| Galactic latitude (°) | -18.4095Ref | Proper motion in δ (mas/yr) | -1.53±0.83Ref |
| X-Ray | NoRef | IR type | SRef | Radio | - |
| X-Ray type | - | J (mag) | - | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | - | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | - | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 14.55Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 14.88Ref | Resolved nebula | - |
| U (mag) | 22.64Ref | WISE W3 (mag) | 12.28Ref | IPmax (eV) | 114Ref |
| B (mag) | 22.82Ref | WISE W4 (mag) | 8.84Ref | [O III] lines | NoRef |
| V (mag) | 21.62Ref | IRAS 12μm (Jy) | - | He II lines | YesRef |
| R (mag) | - | IRAS 25μm (Jy) | - | [Fe VII] lines | NoRef |
| I (mag) | - | IRAS 60μm (Jy) | - | O VI lines | YesRef |
| BP (mag) | 21.04Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 20.35Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 19.02Ref | 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 | CRef | Mass (M⊙) | - | Pulsation | YesRef |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | SRRef |
| IR type | SRef | Luminosity (L⊙) | - | Pulsation period (days) | 142±3Ref |
| Metallicity [Fe/H] | - | Pulsation ephemeris | - |
| Type/Spectral type | WD?Ref | Mass (M⊙) | - | Spin period (min) | - |
| Shell-burning/Accreting-only | shell-burningRef | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | 130000Ref | Luminosity (L⊙) | - | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | - |
This object is identified as an S-type symbiotic star, consisting of an AGB carbon star, and a compact companion, likely a white dwarf. The red giant exhibits characteristics of a semiregular variable, pulsating in the first overtone with a period of 142 days (Kniazev et al., 2009).