CONFIRMED
M31
|
M31SyS J004433.74+414402.8 | IRAS - | GSC2.4.2 NBW9096754 | AAVSO - |
SIMBAD M31SyS J004433.74+414402.8 | Pan-STARRS 158080111405401511 | SAO - | VSX - |
GAIA DR3 381302626698638080 | SkyMapper - | WRAY - | GCVS - |
2MASS J00443375+4144035 | HIP - | Hen - | BD - |
WISE - | TYC - | ESO - | HD - |
Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | M31 SySt-30 (Conf.) |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
Right ascension (°) | 11.1406Ref | Parallax (mas) | - | Reddening E(B-V) (mag) | 0.21±0.02Ref, Note |
Declination (°) | 41.7341Ref | Distance (kpc) | 785±25Ref -, Note |
||
Galactic longitude (°) | 121.5569Ref | Proper motion in α (mas/yr) | - | ||
Galactic latitude (°) | -21.1193Ref | Proper motion in δ (mas/yr) | - |
X-Ray | NoRef | IR type | SRef | Radio | - |
X-Ray type | - | J (mag) | 16.88Ref | Flickering | - |
GALEX FUV (mag) | - | H (mag) | 16.07Ref | Outbursts | - |
GALEX NUV (mag) | - | K (mag) | 15.46Ref | Outburst type | - |
IUE | NoRef | WISE W1 (mag) | - | Jets | - |
FUSE | NoRef | WISE W2 (mag) | - | Resolved nebula | - |
U (mag) | 20.93Ref | WISE W3 (mag) | - | IPmax (eV) | 114Ref |
B (mag) | 21.29Ref | WISE W4 (mag) | - | [O III] lines | YesRef |
V (mag) | 20.82Ref | IRAS 12μm (Jy) | - | He II lines | YesRef |
R (mag) | - | IRAS 25μm (Jy) | - | [Fe VII] lines | YesRef |
I (mag) | 19.07Ref | IRAS 60μm (Jy) | - | O VI lines | YesRef |
BP (mag) | 22.54Ref | IRAS 100μm (Jy) | - | ||
G (mag) | 21.05Ref | AKARI S09 (Jy) | - | ||
RP (mag) | 19.52Ref | 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 | Yes?Ref |
Eff. temperature (K) | - | Radius (R⊙) | - | Type | SR?Ref |
IR type | SRef | Luminosity (L⊙) | - | Pulsation period (days) | ~34?Ref |
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) | 100000Ref | ||||
Upper limit (K) | 145000Ref |
In Bonanos et al. (2003), a variable red star, M31 J004433.7+414403.0, is reported, tentatively classified as a Type II Cepheid. According to Mikołajewska et al. (2014), this star may be M31SyS J004433.74+414402.8, and the 34-day periodicity would then reflect an SR pulsation of the red component.