Wil 1 SySt-1

SUSPECTED WILLMAN 1
 
Constellation
Ursa Major
Equatorial coordinates
α = 10 49 27.858
δ = +51 03 46.160
Galactic coordinates
l = 158.5391°
b = 56.7877°

Suspected 2020Ref
Confirmed -
Symbiotic IR type -
Hot component type -
Outbursts -

Identifiers

Wil 1 SySt-1 IRAS - GSC2.4.2 N93N007813 AAVSO -
SIMBAD [SSI2008] 386 Pan-STARRS 169271623661036075 SAO - VSX -
GAIA DR3 835977725893619712 SkyMapper - WRAY - GCVS -
2MASS - HIP - Hen - BD -
WISE J104928.23+510345.8 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 (°) 162.3661Ref Parallax (mas) 0.373±0.607Ref Reddening E(B-V) (mag) 0.01±0.0Ref, Note
Declination (°) 51.0628Ref Distance (kpc) 1.64Ref, Note, 1.57Ref, Note    
Galactic longitude (°) 158.5391Ref Proper motion in α (mas/yr) 0.03±0.45Ref    
Galactic latitude (°) 56.7877Ref Proper motion in δ (mas/yr) -1.04±0.66Ref    

Observations

X-Ray YesRef IR type - Radio -
X-Ray type βRef J (mag) - Flickering -
GALEX FUV (mag) - H (mag) - Outbursts -
GALEX NUV (mag) - K (mag) - Outburst type -
IUE NoRef WISE W1 (mag) 16.92Ref Jets -
FUSE NoRef WISE W2 (mag) 16.06Ref Resolved nebula -
U (mag) - WISE W3 (mag) 12.82Ref IPmax (eV) -
B (mag) - WISE W4 (mag) 8.73Ref [O III] lines -
V (mag) - IRAS 12μm (Jy) - He II lines -
R (mag) 19.92Ref IRAS 25μm (Jy) - [Fe VII] lines -
I (mag) - IRAS 60μm (Jy) - O VI lines -
BP (mag) 20.63Ref IRAS 100μm (Jy) -
G (mag) 20.37Ref AKARI S09 (Jy) -
RP (mag) 20.07Ref AKARI S18 (Jy) -

Orbit

Orbital period (days) - γ velocity (km/h) -11.70±2.80Ref 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] -1.6Ref     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

This X-ray source was identified as a symbiotic binary by Saeedi & Sasaki (2020).


References


Last updated: November 12, 2020