EG And

CONFIRMED MILKY WAY
 
Constellation
Andromeda
Equatorial coordinates
α = 00 44 37.199
δ = +40 40 45.457
Galactic coordinates
l = 121.5361°
b = -22.1740°

Suspected 1950Ref
Confirmed 1950Ref
Symbiotic IR type SRef
Hot component type accreting-onlyRef
Outbursts -

Identifiers

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

Symbiotic Catalogs

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.)

Position

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
   
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    

Observations

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

Orbit

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 -        

Cool component

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 -

Hot component

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
   
Lower limit (K) -        
Upper limit (K) -        

Links

SIMBAD   CDS Portal   ARAS Database


Notes

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).


References


Last updated: January 13, 2024