CONFIRMED
MILKY WAY
|
K 4-57 | IRAS 22465+5813 | GSC2.4.2 N1DM047711 | AAVSO - |
SIMBAD PN K 4-57 | Pan-STARRS 178183421430233478 | SAO - | VSX 1499426 |
GAIA DR3 2007463560933862016 | SkyMapper - | WRAY - | GCVS - |
2MASS J22483431+5829083 | HIP - | Hen - | BD - |
WISE J224834.29+582908.2 | TYC - | ESO - | HD - |
Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | IPHASJ224834.32+582908.4 (Conf.) |
Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
Right ascension (°) | 342.1430Ref | Parallax (mas) | 0.001±0.069Ref | Reddening E(B-V) (mag) | 0.94±0.03Ref, Note |
Declination (°) | 58.4856Ref | Distance (kpc) | 7.4Ref 6.95Ref, Note, 8.81Ref, Note |
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Galactic longitude (°) | 107.4453Ref | Proper motion in α (mas/yr) | -1.95±0.07Ref | ||
Galactic latitude (°) | -0.6424Ref | Proper motion in δ (mas/yr) | -1.35±0.07Ref |
X-Ray | NoRef | IR type | DRef | Radio | NoRef |
X-Ray type | - | J (mag) | 11.85Ref | Flickering | - |
GALEX FUV (mag) | - | H (mag) | 9.58Ref | Outbursts | - |
GALEX NUV (mag) | - | K (mag) | 7.91Ref | Outburst type | - |
IUE | NoRef | WISE W1 (mag) | 6.00Ref | Jets | - |
FUSE | NoRef | WISE W2 (mag) | 4.97Ref | Resolved nebula | - |
U (mag) | - | WISE W3 (mag) | 3.36Ref | IPmax (eV) | 99Ref |
B (mag) | - | WISE W4 (mag) | 2.26Ref | [O III] lines | YesRef |
V (mag) | - | IRAS 12μm (Jy) | 1.95Ref | He II lines | YesRef |
R (mag) | - | IRAS 25μm (Jy) | 1.26Ref | [Fe VII] lines | YesRef |
I (mag) | - | IRAS 60μm (Jy) | 2.29Ref | O VI lines | NoRef |
BP (mag) | 18.10Ref | IRAS 100μm (Jy) | 31.10Ref | ||
G (mag) | 17.30Ref | AKARI S09 (Jy) | 1.46Ref | ||
RP (mag) | 16.00Ref | AKARI S18 (Jy) | 1.08Ref |
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 | - |
Eff. temperature (K) | - | Radius (R⊙) | - | Type | - |
IR type | DRef | Luminosity (L⊙) | 3950Ref | Pulsation period (days) | - |
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) | 99000Ref | ||||
Upper limit (K) | - |
Listed in the catalog of PNe, however, based on photometry, it is considered a promising symbiotic star candidate of D type, as indicated in Rodríguez-Flores et al. (2014).