IPHAS J194607.52+223112.2

CONFIRMED MILKY WAY
 
Constellation
Vulpecula
Equatorial coordinates
α = 19 46 07.517
δ = +22 31 12.207
Galactic coordinates
l = 59.0687°
b = -1.1272°

Suspected 2010Ref
Confirmed 2010Ref
Symbiotic IR type DRef
Hot component type shell-burningRef
Outbursts -

Identifiers

IPHAS J194607.52+223112.2 IRAS 19439+2223 GSC2.4.2 N1TV131578 AAVSO -
SIMBAD IRAS 19439+2223 Pan-STARRS 135022965313064652 SAO - VSX 238543
GAIA DR3 1827836999154667008 SkyMapper - WRAY - GCVS -
2MASS J19460752+2231122 HIP - Hen - BD -
WISE J194607.52+223112.2 TYC - ESO - HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) - Belzcyński et al. (2001) -
Gaposchkin (1957) - Kenyon (1986) - Akras et al. (2019) IPHASJ194607.52+223112.2 (Conf.)
Boyarchuk (1969) - Vaidis (1988, 1991) -

Position

Right ascension (°) 296.5313Ref Parallax (mas) -0.048±0.086Ref Reddening E(B-V) (mag) 2.4±0.15Ref, Note
Declination (°) 22.5201Ref Distance (kpc) 7.31Ref, Note, 6.15Ref, Note    
Galactic longitude (°) 59.0687Ref Proper motion in α (mas/yr) -2.65±0.09Ref    
Galactic latitude (°) -1.1272Ref Proper motion in δ (mas/yr) -5.05±0.08Ref    

Observations

X-Ray - IR type DRef Radio YesRef
X-Ray type - J (mag) 9.22Ref Flickering -
GALEX FUV (mag) - H (mag) 7.19Ref Outbursts -
GALEX NUV (mag) - K (mag) 5.97Ref Outburst type -
IUE NoRef WISE W1 (mag) 5.11Ref Jets -
FUSE NoRef WISE W2 (mag) 3.92Ref Resolved nebula -
U (mag) - WISE W3 (mag) 1.86Ref IPmax (eV) 114Ref
B (mag) - WISE W4 (mag) 0.75Ref [O III] lines YesRef
V (mag) - IRAS 12μm (Jy) 3.18Ref He II lines YesRef
R (mag) - IRAS 25μm (Jy) 2.53Ref [Fe VII] lines YesRef
I (mag) - IRAS 60μm (Jy) 2.37Ref O VI lines YesRef
BP (mag) 17.02Ref IRAS 100μm (Jy) 47.20Ref
G (mag) 15.26Ref AKARI S09 (Jy) 5.19Ref
RP (mag) 13.72Ref AKARI S18 (Jy) 4.91Ref

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 YesRef
Eff. temperature (K) - Radius (R) - Type MiraRef
IR type DRef Luminosity (L) - Pulsation period (days) 499.7Ref
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


Notes

This object is identified as a D-type symbiotic star based on its 2MASS colors. The continuum exhibits a weak and gradual rise, lacking the absorption bands characteristic of a red giant. Nonetheless, the confirmation of its genuine symbiotic nature is provided by the presence of Raman-scattered emission at 6825 Å (Corradi et al., 2010).


References

  • Corradi, R. L. M., Valentini, M., Munari, U. et al., 2010, A&A, 509, A41, 2010A&A...509A..41C


Last updated: May 20, 2020