CONFIRMED
MILKY WAY
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EG And | IRAS 00418+4024 | GSC2.4.2 NBVE000376 | AAVSO 000-BBC-010 |
SIMBAD V* EG And | Pan-STARRS 156810111551735738 | SAO 36618 | VSX 151 |
GAIA DR3 369176289048301312 | SkyMapper - | WRAY - | GCVS EG And |
2MASS J00443718+4040456 | HIP 3494 | Hen - | BD +39 167 |
WISE J004437.20+404045.5 | TYC 2801-1704-1 | ESO - | HD 4174 |
Bidelman (1954) | - | Allen (1984) | EG And (Conf.) | Belzcyński et al. (2001) | EG And (Conf.) |
Gaposchkin (1957) | - | Kenyon (1986) | EG And (Conf.) | Akras et al. (2019) | EG And (Conf.) |
Boyarchuk (1969) | HD 4174 (Susp.) | Vaidis (1988, 1991) | EG And (Conf.) |
Right ascension (°) | 11.1550Ref | Parallax (mas) | 1.645±0.034Ref | Reddening E(B-V) (mag) | 0.07±0.0Ref, Note |
Declination (°) | 40.6793Ref | Distance (kpc) | 0.4±0.1Ref, 0.59±0.092Ref, 0.4±0.02Ref 0.59Ref, Note, 0.60Ref, Note |
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Galactic longitude (°) | 121.5361Ref | Proper motion in α (mas/yr) | 8.61±0.03Ref | ||
Galactic latitude (°) | -22.1740Ref | Proper motion in δ (mas/yr) | -15.47±0.02Ref |
X-Ray | YesRef | IR type | SRef | Radio | YesRef |
X-Ray type | βRef, δRef | J (mag) | 3.82Ref | Flickering | YesRef |
GALEX FUV (mag) | - | H (mag) | 2.93Ref | Outbursts | - |
GALEX NUV (mag) | - | K (mag) | 2.58Ref | Outburst type | - |
IUE | YesRef | WISE W1 (mag) | 1.11Ref | Jets | - |
FUSE | YesRef | WISE W2 (mag) | 1.39Ref | Resolved nebula | NoRef |
U (mag) | 10.54Ref | WISE W3 (mag) | 2.45Ref | IPmax (eV) | 40.1Ref, 97.1Ref, 114Ref |
B (mag) | 8.93Ref | WISE W4 (mag) | 2.29Ref | [O III] lines | NoRef |
V (mag) | 7.22Ref | IRAS 12μm (Jy) | 4.42Ref | He II lines | NoRef |
R (mag) | - | IRAS 25μm (Jy) | 1.22Ref | [Fe VII] lines | NoRef |
I (mag) | - | IRAS 60μm (Jy) | 1.06Ref | O VI lines | NoRef |
BP (mag) | 7.44Ref | IRAS 100μm (Jy) | 3.62Ref | ||
G (mag) | 6.29Ref | AKARI S09 (Jy) | 5.99Ref | ||
RP (mag) | 5.21Ref | AKARI S18 (Jy) | 1.44Ref |
Orbital period (days) | 482.2±0.6Ref, 481.1±0.4Ref, 482.57±0.53Ref, 483.3±1.3Ref |
γ velocity (km/h) | -94.8Ref, -95.2±0.3Ref, -95.00±0.16Ref, -99.49±1.48Ref |
Size of giant’s orbit (AU) | 0.327Ref, 0.324Ref, 0.323Ref |
Eccentricity | 0.29±0.07Ref, 0.14±0.08Ref, 0Ref, 0Ref |
RV of giant (km/h) | 8.6Ref, 6.35±0.43Ref, 7.32±0.27Ref, 7.34±0.07Ref |
Separation (AU) | - |
Inclination (°) | <40Ref, 78-90Ref, 75Ref |
Inferior conj. of giant (JD) | 2450803.8 | Mass function | 0.032Ref, 0.011Ref, 0.02Ref, 0.0196Ref, 0.019Ref |
Eclipses | YesRef, NoRef, NoRef |
Mass ratio | 3.2-4.4Ref | ||
Orbital ephemeris | - |
Spectral type | M2 IIIRef, M2.4 IIIRef, M3 IIIRef |
Mass (M⊙) | 1.46Ref, 1.1-2.4Ref | Pulsation | - |
Eff. temperature (K) | 3700±100Ref, 3500±150Ref | Radius (R⊙) | 75.2±10Ref, 124Ref | Type | - |
IR type | SRef | Luminosity (L⊙) | 950±250Ref, 2070Ref | Pulsation period (days) | - |
Metallicity [Fe/H] | -0.54±0.05Ref | Pulsation ephemeris | - |
Type/Spectral type | WDRef | Mass (M⊙) | 0.4±0.1Ref, 0.35-0.55Ref | Spin period (min) | - |
Shell-burning/Accreting-only | accreting-onlyRef | Radius (R⊙) | 0.024Ref, 0.003Ref | Accretion disk | - |
Eff. temperature (K) | 20000-40000Ref, 75000Ref, 95000Ref, 80000-95000Ref |
Luminosity (L⊙) | 16Ref, 46Ref, 60Ref, 5-40Ref |
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Lower limit (K) | - | ||||
Upper limit (K) | - |
Suggested to have a magnetic field by Babcock (1950), although this was not confirmed by Slovak (1982). Variability with a period of 40.5 days was detected by Jarzębowski (1964). In Tempesti (1977), similar variability on the timescale of 40-80 days was observed. A period of 470 days was detected by Smith (1980). The UV spectrum shows emission lines such as C IV, He II, Mg II, N V, while the optical spectrum shows Balmer lines, He I, [O III], and [Ne III] (Oliversen et al., 1985). Faint O VI lines in the UV were detected by Crowley et al. (2008).