V343 Ser

CONFIRMED MILKY WAY
 
Constellation
Serpens
Equatorial coordinates
α = 18 12 22.138
δ = -11 40 07.110
Galactic coordinates
l = 18.0899°
b = 3.1895°

Suspected 1973Ref
Confirmed 1978Ref
Symbiotic IR type SRef
Hot component type shell-burningRef
Outbursts YesRef

Identifiers

V343 Ser IRAS 18095-1140 GSC2.4.2 S9K9000108 AAVSO 000-BCX-242
SIMBAD EM* AS 289 Pan-STARRS 93992730924398166 SAO - VSX 34934
GAIA DR3 4156835340974302464 SkyMapper 181222.14-114006.9 WRAY - GCVS V0343 Ser
2MASS J18122215-1140070 HIP - Hen 3-1627 BD -
WISE J181222.14-114007.0 TYC - ESO - HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) AS 289 (Conf.) Belzcyński et al. (2001) AS 289 (Conf.)
Gaposchkin (1957) - Kenyon (1986) AS289 (Conf.) Akras et al. (2019) AS 289 (Conf.)
Boyarchuk (1969) - Vaidis (1988, 1991) F1-11 (Conf.)

Position

Right ascension (°) 273.0922Ref Parallax (mas) 0.303±0.044Ref Reddening E(B-V) (mag) 2.31±0.13Ref, Note
Declination (°) -11.6686Ref Distance (kpc) 2.73Ref, Note, 2.67Ref, Note    
Galactic longitude (°) 18.0899Ref Proper motion in α (mas/yr) -4.18±0.05Ref    
Galactic latitude (°) 3.1895Ref Proper motion in δ (mas/yr) 1.03±0.04Ref    

Observations

X-Ray NoRef IR type SRef Radio YesRef
X-Ray type - J (mag) 6.72Ref Flickering NoRef
GALEX FUV (mag) - H (mag) 5.51Ref Outbursts YesRef
GALEX NUV (mag) - K (mag) 4.99Ref Outburst type -
IUE NoRef WISE W1 (mag) 4.72Ref Jets -
FUSE NoRef WISE W2 (mag) 4.55Ref Resolved nebula -
U (mag) - WISE W3 (mag) 4.35Ref IPmax (eV) 114Ref
B (mag) 15.54Ref WISE W4 (mag) 3.67Ref [O III] lines YesRef
V (mag) 13.51Ref IRAS 12μm (Jy) 1.16Ref He II lines YesRef
R (mag) - IRAS 25μm (Jy) 0.73Ref [Fe VII] lines YesRef
I (mag) - IRAS 60μm (Jy) 6.89Ref O VI lines YesRef
BP (mag) 13.01Ref IRAS 100μm (Jy) 106.00Ref
G (mag) 10.83Ref AKARI S09 (Jy) 1.11Ref
RP (mag) 9.52Ref AKARI S18 (Jy) 0.46Ref

Orbit

Orbital period (days) 450.5±2.2Ref, 511±22Ref γ velocity (km/h) -5.65±0.08Ref Size of giant’s orbit (AU) 0.1Ref
Eccentricity 0.135±0.046Ref RV of giant (km/h) 2.66±0.12Ref Separation (AU) -
Inclination (°) - Inferior conj. of giant (JD) - Mass function 0.00086Ref
Eclipses -     Mass ratio -
Orbital ephemeris Min (V) = 2450724.7 + 511±22 x ERef        

Cool component

Spectral type M3-4 IIIRef, M3.5 IIIRef Mass (M) - Pulsation -
Eff. temperature (K) 3608Ref Radius (R) - Type -
IR type SRef Luminosity (L) - Pulsation period (days) -
Metallicity [Fe/H] -     Pulsation ephemeris -

Hot component

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

Links

SIMBAD   CDS Portal   ARAS Database


Notes

The possible eclipsing nature of the source was suggested by Takamizawa et al. (2001), but it was not supported by Fekel et al. (2001).


References


Last updated: April 18, 2022