LAMOST J004316.72+412226.3
POSSIBLE
M31
Constellation
Andromeda |
Equatorial coordinates
α = 00 43 16.700
δ = +41 22 27.098 |
Galactic coordinates
l = 121.2871°
b = -21.4715° |
Suspected |
2020Ref |
Confirmed |
- |
Symbiotic IR type |
- |
Hot component type |
- |
Outbursts |
- |
|
|
Identifiers
LAMOST J004316.72+412226.3 |
IRAS - |
GSC2.4.2 NBVE083903 |
AAVSO - |
SIMBAD Ford M 31 243 |
Pan-STARRS 157640108195679471 |
SAO - |
VSX - |
GAIA DR3 - |
SkyMapper - |
WRAY - |
GCVS - |
2MASS - |
HIP - |
Hen - |
BD - |
WISE - |
TYC - |
ESO - |
HD - |
Symbiotic Catalogs
Bidelman (1954) |
- |
Allen (1984) |
- |
Belzcyński et al. (2001) |
- |
Gaposchkin (1957) |
- |
Kenyon (1986) |
- |
Akras et al. (2019) |
- |
Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
- |
Position
Right ascension (°) |
10.8196Ref |
Parallax (mas) |
- |
Reddening E(B-V) (mag) |
0.39±0.07Ref, Note |
Declination (°) |
41.3742Ref |
Distance (kpc) |
-, Note |
|
|
Galactic longitude (°) |
121.2871Ref |
Proper motion in α (mas/yr) |
- |
|
|
Galactic latitude (°) |
-21.4715Ref |
Proper motion in δ (mas/yr) |
- |
|
|
Observations
X-Ray |
NoRef |
IR type |
- |
Radio |
- |
X-Ray type |
- |
J (mag) |
- |
Flickering |
- |
GALEX FUV (mag) |
- |
H (mag) |
- |
Outbursts |
- |
GALEX NUV (mag) |
- |
K (mag) |
- |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
- |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
- |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
- |
IPmax (eV) |
35.1Ref |
B (mag) |
- |
WISE W4 (mag) |
- |
[O III] lines |
YesRef |
V (mag) |
- |
IRAS 12μm (Jy) |
- |
He II lines |
NoRef |
R (mag) |
- |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
NoRef |
I (mag) |
- |
IRAS 60μm (Jy) |
- |
O VI lines |
NoRef |
BP (mag) |
- |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
- |
AKARI S09 (Jy) |
- |
|
|
RP (mag) |
- |
AKARI S18 (Jy) |
- |
|
|
Orbit
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 |
- |
|
|
|
|
Cool component
Spectral type |
- |
Mass (M⊙) |
- |
Pulsation |
- |
Eff. temperature (K) |
- |
Radius (R⊙) |
- |
Type |
- |
IR type |
- |
Luminosity (L⊙) |
- |
Pulsation period (days) |
- |
Metallicity [Fe/H] |
- |
|
|
Pulsation ephemeris |
- |
Hot component
Type/Spectral type |
- |
Mass (M⊙) |
- |
Spin period (min) |
- |
Shell-burning/Accreting-only |
- |
Radius (R⊙) |
- |
Accretion disk |
- |
Eff. temperature (K) |
- |
Luminosity (L⊙) |
- |
|
|
Lower limit (K) |
- |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
Notes
Suspected by Zhang et al. (2020), the spectrum of this object shows only Balmer lines and [O III] in emission.
References
- Zhang, M., Chen, B., Huo, Z. et al., 2020, RAA, 20, 6, 097, 2020RAA....20...97Z
Last updated: April 12, 2021