V917 Sco

CONFIRMED MILKY WAY
 
Constellation
Scorpius
Equatorial coordinates
α = 17 48 04.274
δ = -36 08 17.418
Galactic coordinates
l = 354.0997°
b = -4.1693°

Suspected 1978Ref
Confirmed 1978Ref
Symbiotic IR type SRef
Hot component type shell-burningRef
Outbursts YesRef - SyN?Ref

Identifiers

V917 Sco IRAS - GSC2.4.2 S8BJ024716 AAVSO 000-BFL-143
SIMBAD Hen 3-1481 Pan-STARRS - SAO - VSX 33733
GAIA DR3 4040275872793595392 SkyMapper 174804.27-360817.2 WRAY - GCVS V0917 Sco
2MASS J17480427-3608173 HIP - Hen 3-1481 BD -
WISE J174804.27-360817.2 TYC - ESO - HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) Hen 1481 (Conf.) Belzcyński et al. (2001) V917 Sco (Conf.)
Gaposchkin (1957) - Kenyon (1986) V917 Sco (Conf.) Akras et al. (2019) V917 Sco (Conf.)
Boyarchuk (1969) - Vaidis (1988, 1991) V917 Sco (Conf.)

Position

Right ascension (°) 267.0178Ref Parallax (mas) 0.084±0.032Ref Reddening E(B-V) (mag) 0.58±0.02Ref, Note
Declination (°) -36.1382Ref Distance (kpc) 6.79Ref, Note, 6.03Ref, Note    
Galactic longitude (°) 354.0997Ref Proper motion in α (mas/yr) -4.85±0.04Ref    
Galactic latitude (°) -4.1693Ref Proper motion in δ (mas/yr) -5.58±0.02Ref    

Observations

X-Ray NoRef IR type SRef Radio NoRef
X-Ray type - J (mag) 9.42Ref Flickering -
GALEX FUV (mag) - H (mag) 8.30Ref Outbursts YesRef
GALEX NUV (mag) - K (mag) 7.85Ref Outburst type SyN?Ref
IUE NoRef WISE W1 (mag) 7.63Ref Jets -
FUSE NoRef WISE W2 (mag) 7.74Ref Resolved nebula -
U (mag) - WISE W3 (mag) 7.36Ref IPmax (eV) 114Ref
B (mag) 13.90Ref WISE W4 (mag) 6.98Ref [O III] lines YesRef
V (mag) 15.00Ref 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) 15.59Ref IRAS 100μm (Jy) -
G (mag) 13.60Ref AKARI S09 (Jy) -
RP (mag) 12.19Ref 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 M7Ref Mass (M) - Pulsation -
Eff. temperature (K) - Radius (R) - Type -
IR type SRef Luminosity (L) - Pulsation period (days) -
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) -        
Upper limit (K) -        

Links

SIMBAD   CDS Portal   ARAS Database


Notes

Detected in a long-lasting outburst, the light curve is presented in Chaisson (1977).


References


Last updated: May 11, 2020