SUSPECTED M31
Equatorial coordinates
α = 10.422818 ± 0.231300| 00 41 41.476227
δ = 41.052261 ± 0.225000 | +41 03 08.137931 |
|
Constellation |
Andromeda |
Symbiotic IR Type |
|
Spectral Type |
FI |
Magnitude range (V) |
|
Outbursts |
No |
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|
Identifiers
Bol D30 |
GSC – |
TYC – |
WRAY – |
SIMBAD Bol D30 |
HIP – |
SAO – |
Hen – |
BD – |
IRAS – |
GAIA DR2 381164917157806208 |
ESO – |
HD – |
2MASS – |
WISE – |
AAVSO – |
Position
Right ascension (°) |
10.422818 ± 0.231300 |
Parallax (mas) |
– |
Reddening E(B-V) (mag) |
0.225 ± 0.025 |
Declination (°) |
41.052261 ± 0.225000 |
Distance (kpc) |
785.00 ± 25.00 |
|
|
Galactic longitude (°) |
120.953328 ± 0.225000 |
Proper motion in α (mas/yr) |
-0.681 ± 0.499 |
|
|
Galactic latitude (°) |
-21.782042 ± 0.231300 |
Proper motion in δ (mas/yr) |
-1.322 ± 0.502 |
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|
Observations
U (mag) |
19.43 |
X-Ray |
|
Flickering |
|
B (mag) |
19.35 |
X-Ray type |
|
Outbursts |
No |
V (mag) |
19.02 |
IUE |
No |
Type |
|
R (mag) |
18.80 |
IRAS flux at 12 μm (Jy) |
|
IPmax (eV) |
|
I (mag) |
18.53 |
IRAS flux at 25 μm (Jy) |
|
OVI lines |
|
G (mag) |
18.93 |
IRAS flux at 60 μm (Jy) |
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|
|
J (mag) |
|
IRAS flux at 100 μm (Jy) |
|
|
|
H (mag) |
|
WISE W1 (mag) |
14.46 |
|
|
K (mag) |
16.02 |
WISE W2 (mag) |
13.16 |
|
|
L (mag) |
|
WISE W3 (mag) |
10.15 |
|
|
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|
WISE W4 (mag) |
7.44 |
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Radio |
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Radio flux (mJy) |
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Orbit
Orbital period (days) |
|
γ velocity (km/h) |
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Size of giant’s orbit (AU) |
|
Eccentricity |
|
RV of giant (km/h) |
-780 ± 20 |
Separation (AU) |
|
Inclination (°) |
|
Inferior conj. of giant (JD) |
|
Mass function |
|
Ephemeris type |
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Mass ratio |
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Ephemeris T0 (JD) |
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|
|
Cool component
Spectral type |
FI |
Mass (M⊙) |
|
Pulsation |
|
Eff. temperature (K) |
6500 |
Radius (R⊙) |
|
Type |
|
IR type |
|
Luminosity (L⊙) |
15000 |
Pulsation period (days) |
|
Metallicity [Fe/H] |
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|
|
Ephemeris type |
|
|
|
|
|
Ephemeris T0 (JD) |
|
Hot component
Type/Spectra |
|
Mass (M⊙) |
|
Spin period (min) |
|
Eff. temperature (K) |
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Radius (R⊙) |
|
Accretion disk |
|
Lower limit (K) |
|
Luminosity (L⊙) |
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|
Upper limit (K) |
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Links
SIMBAD CDS Portal
Notes
The star has an extremely negative velocity and is probably located in the Giant Stream in M31. Caldwell et al. (2010) speculated that the object could be a symbiotic nova.
References
- Caldwell, N., Morrison, H., Kenyon, S. J., et al., 2010, AJ, 139, 372, 2010AJ….139..372C
Last updated: May 11, 2019 @ 2:41 pm