[JBN2011] 368

SUSPECTED MILKY WAY
 
Constellation
Sagittarius
Equatorial coordinates
α = 17 46 44.335
δ = -26 01 00.180
Galactic coordinates
l = 2.6231°
b = 1.3059°

Suspected 2019Ref
Confirmed -
Symbiotic IR type -
Hot component type -
Outbursts -

Identifiers

[JBN2011] 368 IRAS - GSC2.4.2 S8DX033307 AAVSO -
SIMBAD [JBN2011] 368 Pan-STARRS 76782666847590272 SAO - VSX 476331
GAIA DR3 4067085642765501568 SkyMapper - WRAY - GCVS -
2MASS J17464434-2601002 HIP - Hen - BD -
WISE - TYC - ESO - HD -

Symbiotic Catalogs

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

Position

Right ascension (°) 266.6847Ref Parallax (mas) 0.346±0.127Ref Reddening E(B-V) (mag) 2.32±0.13Ref, Note
Declination (°) -26.0167Ref Distance (kpc) 3.30Ref, Note, 4.53Ref, Note    
Galactic longitude (°) 2.6231Ref Proper motion in α (mas/yr) -2.10±0.15Ref    
Galactic latitude (°) 1.3059Ref Proper motion in δ (mas/yr) -5.80±0.09Ref    

Observations

X-Ray YesRef IR type - Radio -
X-Ray type - J (mag) 14.19Ref Flickering -
GALEX FUV (mag) - H (mag) 13.54Ref Outbursts -
GALEX NUV (mag) - K (mag) 12.69Ref Outburst type -
IUE NoRef WISE W1 (mag) - Jets -
FUSE NoRef WISE W2 (mag) - Resolved nebula -
U (mag) - WISE W3 (mag) - IPmax (eV) -
B (mag) - WISE W4 (mag) - [O III] lines -
V (mag) - IRAS 12μm (Jy) - He II lines -
R (mag) - IRAS 25μm (Jy) - [Fe VII] lines -
I (mag) - IRAS 60μm (Jy) - O VI lines -
BP (mag) 19.76Ref IRAS 100μm (Jy) -
G (mag) 18.12Ref AKARI S09 (Jy) -
RP (mag) 16.81Ref 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 - Mass (M) - Pulsation -
Eff. temperature (K) - Radius (R) - Type -
IR type - Luminosity (L) - Pulsation period (days) -
Metallicity [Fe/H] -     Pulsation ephemeris -

Hot component

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

Links

SIMBAD   CDS Portal


Notes

Classified as a confirmed symbiotic star in the ASAS-SN database (Jayasinghe et al., 2019), this object is likely associated with X-ray source, as indicated by Wevers et al. (2016).


References

  • Jayasinghe, T., Stanek, K. Z., Kochanek, C. S. et al., 2019, MNRAS, 486, 2, 1907, 2019MNRAS.486.1907J
  • Wevers, T., Hodgkin, S. T., Jonker, P. G. et al., 2016, MNRAS, 458, 4, 4530, 2016MNRAS.458.4530W


Last updated: March 17, 2022