M31SyS J004421.89+415125.6

CONFIRMED M31
 
Constellation
Andromeda
Equatorial coordinates
α = 00 44 21.891
δ = +41 51 25.650
Galactic coordinates
l = 121.5213°
b = -20.9953°

Suspected 2014Ref
Confirmed 2014Ref
Symbiotic IR type DRef
Hot component type shell-burningRef
Outbursts -

Identifiers

M31SyS J004421.89+415125.6 IRAS - GSC2.4.2 NBW9012704 AAVSO -
SIMBAD [SCM2012b] HII177 Pan-STARRS 158220110911399133 SAO - VSX -
GAIA DR3 - SkyMapper - WRAY - GCVS -
2MASS J00442178+4151233 HIP - Hen - BD -
WISE - TYC - ESO - HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) - Belzcyński et al. (2001) -
Gaposchkin (1957) - Kenyon (1986) - Akras et al. (2019) M31 SySt-28 (Conf.)
Boyarchuk (1969) - Vaidis (1988, 1991) -

Position

Right ascension (°) 11.0912Ref Parallax (mas) - Reddening E(B-V) (mag) 0.3±0.04Ref, Note
Declination (°) 41.8571Ref Distance (kpc) 785±25Ref
-, Note
   
Galactic longitude (°) 121.5213Ref Proper motion in α (mas/yr) -    
Galactic latitude (°) -20.9953Ref Proper motion in δ (mas/yr) -    

Observations

X-Ray NoRef IR type DRef 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) 20.41Ref WISE W3 (mag) - IPmax (eV) 54.4Ref
B (mag) 21.25Ref WISE W4 (mag) - [O III] lines YesRef
V (mag) 21.27Ref IRAS 12μm (Jy) - He II lines YesRef
R (mag) - IRAS 25μm (Jy) - [Fe VII] lines NoRef
I (mag) 19.91Ref IRAS 60μm (Jy) - O VI lines NoRef
BP (mag) - IRAS 100μm (Jy) -
G (mag) - AKARI S09 (Jy) -
RP (mag) - AKARI S18 (Jy) -

Orbit

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 -        

Cool component

Spectral type MRef Mass (M) - Pulsation YesRef
Eff. temperature (K) - Radius (R) - Type low-amplitude SR?Ref
IR type DRef Luminosity (L) - Pulsation period (days) ~80?Ref
Metallicity [Fe/H] -     Pulsation ephemeris -

Hot component

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) 100000Ref        

Links

SIMBAD   CDS Portal


Notes

Vilardell et al. (2006) report a variable star, M31V J00442188+4151255, coinciding with the position of the symbiotic star within ∼0.1 arcsec. This variable star shows low-amplitude variability with a period P ∼80 days, which is most likely due to SR pulsations of the red giant. This would then indicate that M31SyS J004421.89+415125.6 is not a D-type symbiotic star, as suggested by its position in the [O III] diagram (Mikołajewska et al., 2014).


References


Last updated: January 12, 2019