Hen 3-1103

CONFIRMED MILKY WAY
 
Constellation
Lupus
Equatorial coordinates
α = 15 48 28.273
δ = -44 19 01.558
Galactic coordinates
l = 333.2049°
b = 7.9028°

Suspected 1973Ref
Confirmed 1984Ref
Symbiotic IR type SRef
Hot component type shell-burningRef
Outbursts Yes?Ref

Identifiers

Hen 3-1103 IRAS - GSC2.4.2 S8TR037905 AAVSO 000-BJT-825
SIMBAD WRAY 15-1359 Pan-STARRS - SAO - VSX 241023
GAIA DR3 5989266232815589120 SkyMapper 154828.27-441901.5 WRAY 15-1359 GCVS -
2MASS J15482828-4419015 HIP - Hen 3-1103 BD -
WISE J154828.27-441901.5 TYC - ESO - HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) Hen 1103 (Conf.) Belzcyński et al. (2001) Hen 3-1103 (Conf.)
Gaposchkin (1957) - Kenyon (1986) Hen 1103 (Conf.) Akras et al. (2019) Hen 3-1103 (Conf.)
Boyarchuk (1969) - Vaidis (1988, 1991) VDS 48 (Conf.)

Position

Right ascension (°) 237.1178Ref Parallax (mas) 0.083±0.021Ref Reddening E(B-V) (mag) 0.26±0.01Ref, Note
Declination (°) -44.3171Ref Distance (kpc) 2.3Ref
9.20Ref, Note, 9.38Ref, Note
   
Galactic longitude (°) 333.2049Ref Proper motion in α (mas/yr) -4.54±0.03Ref    
Galactic latitude (°) 7.9028Ref Proper motion in δ (mas/yr) -3.14±0.02Ref    

Observations

X-Ray NoRef IR type SRef Radio NoRef
X-Ray type - J (mag) 9.60Ref Flickering -
GALEX FUV (mag) - H (mag) 8.74Ref Outbursts Yes?Ref
GALEX NUV (mag) - K (mag) 8.36Ref Outburst type -
IUE NoRef WISE W1 (mag) 8.21Ref Jets -
FUSE NoRef WISE W2 (mag) 8.17Ref Resolved nebula NoRef
U (mag) - WISE W3 (mag) 7.63Ref IPmax (eV) 114Ref
B (mag) 14.24Ref WISE W4 (mag) 7.01Ref [O III] lines YesRef
V (mag) 13.39Ref IRAS 12μm (Jy) - He II lines YesRef
R (mag) - IRAS 25μm (Jy) - [Fe VII] lines YesRef
I (mag) - IRAS 60μm (Jy) - O VI lines YesRef
BP (mag) 12.65Ref IRAS 100μm (Jy) -
G (mag) 11.96Ref AKARI S09 (Jy) -
RP (mag) 10.99Ref AKARI S18 (Jy) -

Orbit

Orbital period (days) 698±41Ref 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 Max (V) = 2452211 + 698±41 x ERef        

Cool component

Spectral type M3.5Ref, M1.3Ref 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 WDRef Mass (M) - Spin period (min) -
Shell-burning/Accreting-only shell-burningRef Radius (R) 0.019Ref Accretion disk -
Eff. temperature (K) 183000Ref Luminosity (L) 350Ref    
Lower limit (K) -        
Upper limit (K) -        

Links

SIMBAD   CDS Portal


Notes

There is a suggestion that the object experienced an outburst in 1991, as indicated in the study by Gutiérrez-Moreno et al. (1999).


References


Last updated: November 12, 2020