Sa 3-43

CONFIRMED MILKY WAY
 
Constellation
Ophiucus
Equatorial coordinates
α = 17 17 55.775
δ = -30 01 42.629
Galactic coordinates
l = 355.7867°
b = 4.4474°

Suspected 1984Ref
Confirmed 1992Ref
Symbiotic IR type SRef
Hot component type shell-burningRef
Outbursts -

Identifiers

Sa 3-43 IRAS - GSC2.4.2 S8HO121700 AAVSO 000-BJT-831
SIMBAD PN Sa 3-43 Pan-STARRS 71962594824056097 SAO - VSX 241035
GAIA DR3 4059208981986040192 SkyMapper 171755.78-300142.4 WRAY - GCVS -
2MASS J17175578-3001425 HIP - Hen - BD -
WISE J171755.77-300142.5 TYC - ESO - HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) Sa3-43 (Susp.) Belzcyński et al. (2001) Sa 3-43 (Conf.)
Gaposchkin (1957) - Kenyon (1986) Sa 3-43 (Susp.) Akras et al. (2019) PN Sa 3-43 (Conf.)
Boyarchuk (1969) - Vaidis (1988, 1991) Sa 3-43 (Conf.)

Position

Right ascension (°) 259.4824Ref Parallax (mas) 0.197±0.023Ref Reddening E(B-V) (mag) 0.96±0.03Ref, Note
Declination (°) -30.0285Ref Distance (kpc) 3.96Ref, Note, 3.88Ref, Note    
Galactic longitude (°) 355.7867Ref Proper motion in α (mas/yr) -4.41±0.03Ref    
Galactic latitude (°) 4.4474Ref Proper motion in δ (mas/yr) -5.22±0.02Ref    

Observations

X-Ray NoRef IR type SRef Radio NoRef
X-Ray type - J (mag) 9.48Ref Flickering -
GALEX FUV (mag) - H (mag) 8.23Ref Outbursts -
GALEX NUV (mag) - K (mag) 7.84Ref Outburst type -
IUE NoRef WISE W1 (mag) 7.54Ref Jets -
FUSE NoRef WISE W2 (mag) 7.51Ref Resolved nebula -
U (mag) - WISE W3 (mag) 7.28Ref IPmax (eV) 54.4Ref
B (mag) 17.13Ref WISE W4 (mag) 6.77Ref [O III] lines NoRef
V (mag) 14.95Ref IRAS 12μm (Jy) - He II lines YesRef
R (mag) 13.84Ref IRAS 25μm (Jy) - [Fe VII] lines NoRef
I (mag) 11.62Ref IRAS 60μm (Jy) - O VI lines NoRef
BP (mag) 15.13Ref IRAS 100μm (Jy) -
G (mag) 13.24Ref AKARI S09 (Jy) -
RP (mag) 11.94Ref AKARI S18 (Jy) -

Orbit

Orbital period (days) - γ velocity (km/h) -69.84±1.07Ref 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 M0Ref 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) 92000Ref Luminosity (L) -    
Lower limit (K) -        
Upper limit (K) 86000Ref        

Links

SIMBAD   CDS Portal


Notes

Suspected by Allen (1984), it was later confirmed to be a symbiotic star based on spectroscopic observations, as reported in Gutiérrez-Moreno et al. (1992).


References


Last updated: December 1, 2021