CONFIRMED M31
Equatorial coordinates
α = 10.894874 ± 0.751300 | 00 43 34.769677
δ = 41.579937 ± 0.561100 | +41 34 47.774896 |
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Constellation |
Andromeda |
Symbiotic IR Type |
S |
Spectral Type |
M |
Magnitude range (V) |
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Outbursts |
No |
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Identifiers
Position
Right ascension (°) |
10.894874 ± 0.751300 |
Parallax (mas) |
– |
Reddening E(B-V) (mag) |
0.250 ± 0.015 |
Declination (°) |
41.579937 ± 0.561100 |
Distance (kpc) |
785.00 ± 25.00 |
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Galactic longitude (°) |
121.355045 ± 0.561100 |
Proper motion in α (mas/yr) |
– |
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Galactic latitude (°) |
-21.267751 ± 0.751300 |
Proper motion in δ (mas/yr) |
– |
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Observations
U (mag) |
20.63 |
X-Ray |
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Flickering |
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B (mag) |
21.30 |
X-Ray type |
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Outbursts |
No |
V (mag) |
20.91 |
IUE |
No |
Type |
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R (mag) |
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IRAS flux at 12 μm (Jy) |
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IPmax (eV) |
41.0 |
I (mag) |
19.56 |
IRAS flux at 25 μm (Jy) |
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OVI lines |
No |
G (mag) |
20.39 |
IRAS flux at 60 μm (Jy) |
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J (mag) |
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IRAS flux at 100 μm (Jy) |
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H (mag) |
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WISE W1 (mag) |
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K (mag) |
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WISE W2 (mag) |
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L (mag) |
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WISE W3 (mag) |
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WISE W4 (mag) |
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Radio |
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Radio flux (mJy) |
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Orbit
Orbital period (days) |
∼260? |
γ velocity (km/h) |
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Size of giant’s orbit (AU) |
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Eccentricity |
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RV of giant (km/h) |
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Separation (AU) |
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Inclination (°) |
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Inferior conj. of giant (JD) |
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Mass function |
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Ephemeris type |
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Mass ratio |
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Ephemeris T0 (JD) |
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Cool component
Spectral type |
M |
Mass (M⊙) |
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Pulsation |
Yes? |
Eff. temperature (K) |
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Radius (R⊙) |
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Type |
Low-amplitude SR pulsations? |
IR type |
S |
Luminosity (L⊙) |
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Pulsation period (days) |
∼83? |
Metallicity [Fe/H] |
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Ephemeris type |
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Ephemeris T0 (JD) |
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Hot component
Type/Spectra |
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Mass (M⊙) |
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Spin period (min) |
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Eff. temperature (K) |
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Radius (R⊙) |
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Accretion disk |
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Lower limit (K) |
41000 |
Luminosity (L⊙) |
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Upper limit (K) |
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Links
SIMBAD CDS Portal
Notes
There is a red variable, [PAC] 46291, with P ∼260 d, which couldbe the same object (Mikołajewska et al., 2014).
References
- Mikołajewska, J., Caldwell, N., Shara, M. M., 2014, MNRAS, 444, 586, 2014MNRAS.444..586M
Last updated: Jan 12, 2019 @ 3:54 pm