[O2006] QSS 10

SUSPECTED M31
 
Constellation
Andromeda
Equatorial coordinates
α = 00 42 38.770
δ = +41 15 26.880
Galactic coordinates
l = 121.1552°
b = -21.5840°

Suspected 2014Ref
Confirmed -
Symbiotic IR type -
Hot component type -
Outbursts -

Identifiers

[O2006] QSS 10 IRAS - GSC2.4.2 NBVE062080 AAVSO -
SIMBAD [O2006] QSS 10 Pan-STARRS - SAO - VSX -
GAIA DR3 - SkyMapper - WRAY - GCVS -
2MASS - 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) -
Boyarchuk (1969) - Vaidis (1988, 1991) -

Position

Right ascension (°) 10.6615Ref Parallax (mas) - Reddening E(B-V) (mag) 0.48±0.1Ref, Note
Declination (°) 41.2575Ref Distance (kpc) 785±25Ref
-, Note
   
Galactic longitude (°) 121.1552Ref Proper motion in α (mas/yr) -    
Galactic latitude (°) -21.5840Ref Proper motion in δ (mas/yr) -    

Observations

X-Ray YesRef 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) - WISE W3 (mag) - IPmax (eV) -
B (mag) - WISE W4 (mag) - [O III] lines -
V (mag) - IRAS 12μm (Jy) - He II lines -
R (mag) - IRAS 25μm (Jy) - [Fe VII] lines -
I (mag) - IRAS 60μm (Jy) - O VI lines -
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 - Mass (M) - Pulsation -
Eff. temperature (K) - Radius (R) - Type -
IR type - Luminosity (L) - Pulsation period (days) -
Metallicity [Fe/H] -     Pulsation ephemeris -

Hot component

Type/Spectral type - Mass (M) - Spin period (min) -
Shell-burning/Accreting-only - Radius (R) - Accretion disk -
Eff. temperature (K) - Luminosity (L) -    
Lower limit (K) -        
Upper limit (K) -        

Links

SIMBAD   CDS Portal


Notes

Identified as an X-ray source in M31, Chiosi et al. (2014) suspected its symbiotic nature. However, the object is located in a rather crowded field, and, moreover, the X-ray luminosity is quite low (and variable?), which is not consistent with hydrogen burning.


References

  • Chiosi, E., Orio, M., Bernardini, F. et al., 2014, MNRAS, 443, 2, 1821, 2014MNRAS.443.1821C
  • Kong, A. K. H., Garcia, M. R., Primini, F. A. et al., 2002, ApJ, 577, 2, 738, 2002ApJ...577..738K


Last updated: May 11, 2019