CONFIRMED
M33
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M33SyS J013510.81+305146.8 | IRAS - | GSC2.4.2 NBXX051147 | AAVSO - |
SIMBAD M33SyS J013510.81+305146.8 | Pan-STARRS 145030237949416180 | SAO - | VSX - |
GAIA DR3 - | SkyMapper - | WRAY - | GCVS - |
2MASS - | HIP - | Hen - | BD - |
WISE - | TYC - | ESO - | HD - |
Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | M33 SySt-12 (Conf.) |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
Right ascension (°) | 23.7950Ref | Parallax (mas) | - | Reddening E(B-V) (mag) | 0.04±0.0Ref, Note |
Declination (°) | 30.8629Ref | Distance (kpc) | 847±60Ref -, Note |
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Galactic longitude (°) | 133.8922Ref | Proper motion in α (mas/yr) | - | ||
Galactic latitude (°) | -31.0762Ref | 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) | - | Jets | - |
FUSE | NoRef | WISE W2 (mag) | - | Resolved nebula | - |
U (mag) | 22.66Ref | WISE W3 (mag) | - | IPmax (eV) | 54.4Ref |
B (mag) | 23.29Ref | WISE W4 (mag) | - | [O III] lines | YesRef |
V (mag) | 22.47Ref | IRAS 12μm (Jy) | - | He II lines | YesRef |
R (mag) | 21.14Ref | IRAS 25μm (Jy) | - | [Fe VII] lines | NoRef |
I (mag) | 20.29Ref | 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 | M4Ref | Mass (M⊙) | - | Pulsation | YesRef |
Eff. temperature (K) | - | Radius (R⊙) | - | Type | low-amplitude SRRef |
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) | 54000Ref | ||||
Upper limit (K) | 127000Ref |
M33SyS J013510.81+305146.8 exhibits clearly detectable ZrO bands, indicating some s-process enrichment. The variability of M33SyS J013510.81+305146.8, especially in the g and r bands, is likely due to orbital motion, with the low-amplitude SR pulsation of the red giant dominating in the i band (Mikołajewska et al., 2017).