AS 221

CONFIRMED MILKY WAY
 
Constellation
Scorpius
Equatorial coordinates
α = 17 12 12.859
δ = -32 37 46.805
Galactic coordinates
l = 352.9524°
b = 3.9330°

Suspected 1950Ref
Confirmed 1978Ref
Symbiotic IR type SRef, DRef
Hot component type shell-burningRef
Outbursts -

Identifiers

AS 221 IRAS - GSC2.4.2 S8GS312378 AAVSO 000-BJX-981
SIMBAD EM* AS 221 Pan-STARRS - SAO - VSX 46895
GAIA DR3 5979902864926562176 SkyMapper 171212.86-323746.6 WRAY 15-1637 GCVS -
2MASS J17121286-3237469 HIP - Hen 3-1348 BD -
WISE J171212.85-323746.8 TYC - ESO 392-4 HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) AS 221 (Conf.) Belzcyński et al. (2001) AS 221 (Conf.)
Gaposchkin (1957) - Kenyon (1986) AS 221 (Conf.) Akras et al. (2019) AS 221 (Conf.)
Boyarchuk (1969) MHa 276-12 (Susp.) Vaidis (1988, 1991) NSV 8271 (Conf.)

Position

Right ascension (°) 258.0536Ref Parallax (mas) 0.062±0.033Ref Reddening E(B-V) (mag) 0.94±0.01Ref, Note
Declination (°) -32.6297Ref Distance (kpc) 5Ref, 4Ref
7.39Ref, Note, 7.29Ref, Note
   
Galactic longitude (°) 352.9524Ref Proper motion in α (mas/yr) -2.33±0.04Ref    
Galactic latitude (°) 3.9330Ref Proper motion in δ (mas/yr) -3.60±0.03Ref    

Observations

X-Ray NoRef IR type SRef, DRef Radio YesRef
X-Ray type - J (mag) 12.14Ref Flickering -
GALEX FUV (mag) - H (mag) 10.10Ref Outbursts -
GALEX NUV (mag) - K (mag) 8.73Ref Outburst type -
IUE NoRef WISE W1 (mag) 7.18Ref Jets -
FUSE NoRef WISE W2 (mag) 7.13Ref Resolved nebula -
U (mag) - WISE W3 (mag) 4.62Ref IPmax (eV) 114Ref
B (mag) - WISE W4 (mag) 3.69Ref [O III] lines YesRef
V (mag) 16.00Ref IRAS 12μm (Jy) - He II lines YesRef
R (mag) - IRAS 25μm (Jy) - [Fe VII] lines YesRef
I (mag) - IRAS 60μm (Jy) - O VI lines YesRef
BP (mag) 16.01Ref IRAS 100μm (Jy) -
G (mag) 14.19Ref AKARI S09 (Jy) 0.48Ref
RP (mag) 12.77Ref AKARI S18 (Jy) 0.30Ref

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 M4 IIIRef, M4 IIIRef,
M1 IIIRef, M7.5 IIIRef
Mass (M) - Pulsation -
Eff. temperature (K) 3560Ref Radius (R) - Type -
IR type SRef, DRef Luminosity (L) 5923Ref Pulsation period (days) -
Metallicity [Fe/H] -     Pulsation ephemeris -

Hot component

Type/Spectral type WDRef Mass (M) - Spin period (min) -
Shell-burning/Accreting-only shell-burningRef Radius (R) - Accretion disk -
Eff. temperature (K) - Luminosity (L) 1800Ref    
Lower limit (K) 114000Ref        
Upper limit (K) -        

Links

SIMBAD   CDS Portal


Notes

Merrill & Burwell (1950) reported the presence of [Fe VII] lines for the star. It was also suspected as a symbiotic star by Allen & Glass (1974). Stenholm & Acker (1987) reported the detection of emission lines with ionization potentials extending up to 114 eV.


References


Last updated: April 17, 2022