CONFIRMED
MILKY WAY
|
LT Del | IRAS - | GSC2.4.2 N2PF000443 | AAVSO 000-BCV-823 |
SIMBAD V* LT Del | Pan-STARRS 132223089885149651 | SAO - | VSX 13555 |
GAIA DR3 1817300516637652352 | SkyMapper - | WRAY - | GCVS LT Del |
2MASS J20355722+2011275 | HIP - | Hen 2-467 | BD - |
WISE J203557.23+201127.4 | TYC - | ESO - | HD - |
Bidelman (1954) | - | Allen (1984) | He2-467 (Conf.) | Belzcyński et al. (2001) | LT Del (Conf.) |
Gaposchkin (1957) | - | Kenyon (1986) | He2-467 (Conf.) | Akras et al. (2019) | LT Del (Conf.) |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | LT Del (Conf.) |
Right ascension (°) | 308.9885Ref | Parallax (mas) | 0.085±0.015Ref | Reddening E(B-V) (mag) | 0.08±0.0Ref, Note |
Declination (°) | 20.1910Ref | Distance (kpc) | 2Ref, 3.9Ref 9.87Ref, Note, 9.43Ref, Note |
||
Galactic longitude (°) | 63.3967Ref | Proper motion in α (mas/yr) | -0.54±0.01Ref | ||
Galactic latitude (°) | -12.1503Ref | Proper motion in δ (mas/yr) | -2.60±0.01Ref |
X-Ray | NoRef | IR type | SRef | Radio | NoRef |
X-Ray type | - | J (mag) | 10.46Ref | Flickering | NoRef |
GALEX FUV (mag) | 15.94Ref | H (mag) | 9.67Ref | Outbursts | YesRef |
GALEX NUV (mag) | 16.38Ref | K (mag) | 9.50Ref | Outburst type | Z AndRef |
IUE | NoRef | WISE W1 (mag) | 9.32Ref | Jets | - |
FUSE | NoRef | WISE W2 (mag) | 9.34Ref | Resolved nebula | No Ref |
U (mag) | - | WISE W3 (mag) | 8.95Ref | IPmax (eV) | 77.5 (UV)Ref, 54.4Ref |
B (mag) | - | WISE W4 (mag) | 8.16Ref | [O III] lines | YesRef |
V (mag) | - | IRAS 12μm (Jy) | - | He II lines | YesRef |
R (mag) | - | IRAS 25μm (Jy) | - | [Fe VII] lines | NoRef |
I (mag) | - | IRAS 60μm (Jy) | - | O VI lines | NoRef |
BP (mag) | 13.40Ref | IRAS 100μm (Jy) | - | ||
G (mag) | 12.60Ref | AKARI S09 (Jy) | - | ||
RP (mag) | 11.71Ref | AKARI S18 (Jy) | - |
Orbital period (days) | 478.5±2.5Ref, 465.6Ref, 462.81±6.88Ref |
γ velocity (km/h) | -100.54±2.66Ref | Size of giant’s orbit (AU) | - |
Eccentricity | 0.4±0.1Ref | RV of giant (km/h) | - | Separation (AU) | - |
Inclination (°) | - | Inferior conj. of giant (JD) | - | Mass function | - |
Eclipses | NoRef | Mass ratio | 1.63Ref | ||
Orbital ephemeris | Min (U) = 2445910 + 478.5±2.5Ref, Min (B) = 2440493 + 465.6 x ERef |
Spectral type | G6 IIIRef, K0 IIIRef | Mass (M⊙) | 1Ref, 0.93Ref | Pulsation | - |
Eff. temperature (K) | 4400±150Ref | Radius (R⊙) | 30Ref, 46Ref | Type | - |
IR type | SRef | Luminosity (L⊙) | 140Ref, 230Ref, 700Ref |
Pulsation period (days) | - |
Metallicity [Fe/H] | -1.1±0.1Ref | Pulsation ephemeris | - |
Type/Spectral type | WDRef | Mass (M⊙) | 0.57Ref | Spin period (min) | - |
Shell-burning/Accreting-only | shell-burningRef | Radius (R⊙) | 0.06Ref | Accretion disk | - |
Eff. temperature (K) | 200000Ref, 105000-130000Ref | Luminosity (L⊙) | 5400Ref | ||
Lower limit (K) | - | ||||
Upper limit (K) | - |
The optical spectrum of this object exhibits emission lines with ionization potentials of up to 54 eV, including He II, as observed by Munari & Buson (1992). Additionally, UV spectra revealed N V lines. Notably, the object displays both hot and cool outbursts similar to AG Dra, as reported by Ikonnikova et al. (2019).