[LDB2002] 701

SUSPECTED NGC 6822  

Equatorial coordinates
α =  296.285640 | 19 45 08.550000
δ =  -14.740750 | -14 44 26.700000
 
Constellation Sagittarius
Symbiotic IR Type S
Spectral Type C
Magnitude range (V)  
Outbursts No

Identifiers

[LDB2002] 701 GSC TYC WRAY
SIMBAD [LDB2002] 701 HIP SAO Hen
BD – IRAS  GAIA DR2 ESO
HD 2MASS  WISE  AAVSO

Position

Right ascension (°) 296.285640ref Parallax (mas) Reddening E(B-V) (mag) 0.189 ± 0.007ref
Declination (°) -14.740750ref Distance (kpc) 500.00 ± 10.00ref    
Galactic longitude (°) 25.418576ref Proper motion in α (mas/yr)    
Galactic latitude (°) -18.413336ref Proper motion in δ (mas/yr)    

Observations

U (mag)   X-Ray   Flickering  
B (mag)   X-Ray type   Outbursts No
V (mag)   IUE No Type  
R (mag)   IRAS flux at 12 μm (Jy)   IPmax (eV)  
I (mag)   IRAS flux at 25 μm (Jy)   OVI lines  
G (mag)   IRAS flux at 60 μm (Jy)      
J (mag) 16.67ref IRAS flux at 100 μm (Jy)      
H (mag) 15.62ref WISE W1 (mag)      
K (mag) 15.09ref WISE W2 (mag)      
L (mag)   WISE W3 (mag)      
    WISE W4 (mag)      
    Radio      
    Radio flux (mJy)      

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  
Ephemeris type       Mass ratio  
Ephemeris T(JD)          

Cool component

Spectral type Cref Mass (M)   Pulsation  
Eff. temperature (K)   Radius (R)   Type  
IR type Sref Luminosity (L)   Pulsation period (days)  
Metallicity [Fe/H]       Ephemeris type  
        Ephemeris T(JD)  

Hot component

Type/Spectra   Mass (M)   Spin period (min)  
Eff. temperature (K)   Radius (R)   Accretion disk  
Lower limit (K)   Luminosity (L)      
Upper limit (K)          

Links

SIMBAD     CDS Portal


Notes

It was suspected to be a symbiotic star based on its spectra by Sibbons et al. (2015).


References

  • Sibbons, L. F., Ryan, S. G., Napiwotzki, R., et al., 2015, A&A, 574, A102, 2015A&A…574A.102S

Last updated: May 13, 2019 @ 11:17 am