CONFIRMED
MILKY WAY
|
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 - |
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) | - |
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 |
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 |
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 | - |
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 | - |
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) | - |
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).