V1196 Sco

CONFIRMED MILKY WAY
 
Constellation
Scorpius
Equatorial coordinates
α = 16 51 20.396
δ = -26 00 26.861
Galactic coordinates
l = 355.5145°
b = 11.5536°

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

Identifiers

V1196 Sco IRAS 16482-2555 GSC2.4.2 S8F9000250 AAVSO 000-BFQ-793
SIMBAD EM* AS 210 Pan-STARRS 76792528350111376 SAO - VSX 136725
GAIA DR3 6034584803576395648 SkyMapper 165120.39-260026.6 WRAY 16-237 GCVS V1196 Sco
2MASS J16512040-2600267 HIP - Hen 3-1265 BD -
WISE J165120.39-260027.0 TYC - ESO - HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) AS 210 (Conf.) Belzcyński et al. (2001) AS 210 (Conf.)
Gaposchkin (1957) - Kenyon (1986) AS 210 (Conf.) Akras et al. (2019) AS 210 (Conf.)
Boyarchuk (1969) MHa 276-52 (Susp.) Vaidis (1988, 1991) MHA 276-52 (Conf.)

Position

Right ascension (°) 252.8350Ref Parallax (mas) 0.128±0.041Ref Reddening E(B-V) (mag) 0.23±0.0Ref, Note
Declination (°) -26.0075Ref Distance (kpc) 5.6Ref
7.44Ref, Note, 5.46Ref, Note
   
Galactic longitude (°) 355.5145Ref Proper motion in α (mas/yr) -7.49±0.05Ref    
Galactic latitude (°) 11.5536Ref Proper motion in δ (mas/yr) -2.37±0.04Ref    

Observations

X-Ray NoRef IR type DRef Radio YesRef
X-Ray type - J (mag) 9.09Ref Flickering -
GALEX FUV (mag) - H (mag) 7.56Ref Outbursts -
GALEX NUV (mag) - K (mag) 6.26Ref Outburst type -
IUE YesRef WISE W1 (mag) 4.99Ref Jets -
FUSE YesRef WISE W2 (mag) 3.71Ref Resolved nebula NoRef
U (mag) - WISE W3 (mag) 2.90Ref IPmax (eV) 114Ref
B (mag) 14.36Ref WISE W4 (mag) 2.50Ref [O III] lines YesRef
V (mag) 13.75Ref IRAS 12μm (Jy) 3.93Ref He II lines YesRef
R (mag) - IRAS 25μm (Jy) 1.21Ref [Fe VII] lines NoRef
I (mag) - IRAS 60μm (Jy) 0.40Ref O VI lines YesRef
BP (mag) 12.94Ref IRAS 100μm (Jy) 2.10Ref
G (mag) 12.28Ref AKARI S09 (Jy) 2.90Ref
RP (mag) 11.06Ref AKARI S18 (Jy) 1.50Ref

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 C3Ref Mass (M) - Pulsation YesRef
Eff. temperature (K) - Radius (R) - Type MiraRef
IR type DRef Luminosity (L) - Pulsation period (days) 423±7Ref
Metallicity [Fe/H] -     Pulsation ephemeris Max (JHKL) = 2446162 + 423±7 x ERef

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) -        
Upper limit (K) -        

Links

SIMBAD   CDS Portal   ARAS Database


Notes

Carbon Mira, as reported by Merrill & Burwell (1950), exhibits [Fe VII] lines. It was classified as a potential symbiotic star by Wilde (1965) and Henize (1967).


References


Last updated: April 17, 2022