OGLE BLG654.20 36111

POSSIBLE MILKY WAY
 
Constellation
Ophiucus
Equatorial coordinates
α = 17 36 20.191
δ = -29 33 38.976
Galactic coordinates
l = 358.3977°
b = 1.3870°

Suspected 2014Ref
Confirmed -
Symbiotic IR type S?Ref
Hot component type accreting-only?Ref
Outbursts -

Identifiers

OGLE BLG654.20 36111 IRAS - GSC2.4.2 S8DK012199 AAVSO -
SIMBAD OGLE BLG654.20 36111 Pan-STARRS 72522640841257303 SAO - VSX 285556
GAIA DR3 4060066227422719872 SkyMapper 173620.14-293338.6 WRAY - GCVS -
2MASS J17362020-2933389 HIP - Hen - BD -
WISE J173620.11-293338.4 TYC - ESO - HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) - Belzcyński et al. (2001) -
Gaposchkin (1957) - Kenyon (1986) - Akras et al. (2019) CXOGBS J173620.2-293338 (Susp.)
Boyarchuk (1969) - Vaidis (1988, 1991) -

Position

Right ascension (°) 264.0841Ref Parallax (mas) 0.368±0.114Ref Reddening E(B-V) (mag) 2.37±0.09Ref, Note
Declination (°) -29.5608Ref Distance (kpc) 8Ref
3.74Ref, Note, 3.72Ref, Note
   
Galactic longitude (°) 358.3977Ref Proper motion in α (mas/yr) -4.17±0.15Ref    
Galactic latitude (°) 1.3870Ref Proper motion in δ (mas/yr) 7.89±0.11Ref    

Observations

X-Ray YesRef IR type S?Ref Radio -
X-Ray type γ?Ref J (mag) 11.54Ref Flickering -
GALEX FUV (mag) - H (mag) 10.13Ref Outbursts -
GALEX NUV (mag) - K (mag) 9.65Ref Outburst type -
IUE NoRef WISE W1 (mag) 8.83Ref Jets -
FUSE NoRef WISE W2 (mag) 8.84Ref Resolved nebula -
U (mag) - WISE W3 (mag) 8.59Ref IPmax (eV) No linesRef
B (mag) - WISE W4 (mag) 7.37Ref [O III] lines NoRef
V (mag) - IRAS 12μm (Jy) - He II lines NoRef
R (mag) - IRAS 25μm (Jy) - [Fe VII] lines NoRef
I (mag) 15.16Ref IRAS 60μm (Jy) - O VI lines NoRef
BP (mag) 19.66Ref IRAS 100μm (Jy) -
G (mag) 16.68Ref AKARI S09 (Jy) -
RP (mag) 15.09Ref 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 C-RRef Mass (M) - Pulsation -
Eff. temperature (K) - Radius (R) - Type -
IR type S?Ref Luminosity (L) - Pulsation period (days) -
Metallicity [Fe/H] -     Pulsation ephemeris -

Hot component

Type/Spectral type WD/NS?Ref, NS?Ref Mass (M) - Spin period (min) -
Shell-burning/Accreting-only accreting-only?Ref Radius (R) - Accretion disk -
Eff. temperature (K) - Luminosity (L) -    
Lower limit (K) -        
Upper limit (K) -        

Links

SIMBAD   CDS Portal


Notes

Suspected of having a symbiotic nature by Hynes et al. (2014) and Wetuski et al. (2021), this star was discovered as an X-ray source with a carbon star identified as its optical counterpart.


References

  • Hynes, R. I., Torres, M. A. P., Heinke, C. O. et al., 2014, ApJ, 780, 1, 11, 2014ApJ...780...11H
  • Wetuski, J., Hynes, R. I., Maccarone, T. J. et al., 2021, MNRAS, 506, 4, 5619, 2021MNRAS.506.5619W


Last updated: November 5, 2019