XMMU J174654.1-291542

SUSPECTED MILKY WAY
 
Constellation
Sagittarius
Equatorial coordinates
α = 17 46 54.374
δ = -29 15 41.080
Galactic coordinates
l = 359.8682°
b = -0.4091°

Suspected 2012Ref
Confirmed -
Symbiotic IR type -
Hot component type -
Outbursts -

Identifiers

XMMU J174654.1-291542 IRAS - GSC2.4.2 S8DO296576 AAVSO -
SIMBAD XMMU J174654.1-291542 Pan-STARRS - SAO - VSX -
GAIA DR3 - SkyMapper - WRAY - GCVS -
2MASS J17465437-2915410 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 (°) 266.7266Ref Parallax (mas) - Reddening E(B-V) (mag) 14.48±2.66Ref, Note
Declination (°) -29.2614Ref Distance (kpc) 6Ref
-, Note
   
Galactic longitude (°) 359.8682Ref Proper motion in α (mas/yr) -    
Galactic latitude (°) -0.4091Ref Proper motion in δ (mas/yr) -    

Observations

X-Ray YesRef IR type - Radio -
X-Ray type γ or δ?Ref J (mag) 16.43Ref Flickering -
GALEX FUV (mag) - H (mag) 12.92Ref Outbursts -
GALEX NUV (mag) - K (mag) 11.58Ref 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) - IRAS 100μm (Jy) -
G (mag) - AKARI S09 (Jy) -
RP (mag) - 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

Detected as an X-ray source, there might be an infrared counterpart (Degenaar et al., 2012).


References


Last updated: May 11, 2020