CONFIRMED
IC10
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| IC10 SySt-1 | IRAS - | GSC2.4.2 NALA114494 | AAVSO - |
| SIMBAD NAME IC10-SySt-01 | Pan-STARRS 179170051397985962 | SAO - | VSX - |
| GAIA DR3 - | SkyMapper - | WRAY - | GCVS - |
| 2MASS - | HIP - | Hen - | BD - |
| WISE J002033.57+591845.7 | TYC - | ESO - | HD - |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | IC10 SySt-1 (Conf.) |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
| Right ascension (°) | 5.1400Ref | Parallax (mas) | - | Reddening E(B-V) (mag) | 1.08±0.16Ref, Note |
| Declination (°) | 59.3128Ref | Distance (kpc) | 660±60Ref -, Note |
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| Galactic longitude (°) | 118.9945Ref | Proper motion in α (mas/yr) | - | ||
| Galactic latitude (°) | -3.3227Ref | Proper motion in δ (mas/yr) | - |
| X-Ray | NoRef | IR type | - | 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) | 13.77Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 13.53Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 12.68Ref | IPmax (eV) | 35.1Ref |
| B (mag) | 26.79Ref | WISE W4 (mag) | 9.36Ref | [O III] lines | YesRef |
| V (mag) | 24.62Ref | IRAS 12μm (Jy) | - | He II lines | NoRef |
| R (mag) | 21.85Ref | IRAS 25μm (Jy) | - | [Fe VII] lines | NoRef |
| I (mag) | 19.46Ref | IRAS 60μm (Jy) | - | O VI lines | NoRef |
| BP (mag) | - | IRAS 100μm (Jy) | - | ||
| G (mag) | - | AKARI S09 (Jy) | - | ||
| RP (mag) | - | 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 | M8 IIIRef | Mass (M⊙) | - | Pulsation | - |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | - |
| IR type | - | Luminosity (L⊙) | - | Pulsation period (days) | - |
| Metallicity [Fe/H] | - | Pulsation ephemeris | - |
| Type/Spectral type | - | Mass (M⊙) | - | Spin period (min) | - |
| Shell-burning/Accreting-only | shell-burningRef | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | 35000Ref | ||||
| Upper limit (K) | 90000Ref |
The first known symbiotic star in IC10, its spectrum of the cool component well matches that of solar neighborhood M8 III giants. The observed emission lines belong to the Balmer series, [S II], [N II], and [O III] (Gonçalves et al., 2008). They also noted that the spectrum of this system is an almost perfect copy of that of Hen 2-147, a Galactic symbiotic star hosting Mira cool component.