SUSPECTED LMC
Equatorial coordinates
α = 83.377143 ± 0.347400 | 05 33 30.514386
δ = -69.874165 ± 0.382500 | -69 52 26.992786 |
|
Constellation |
Dorado |
Symbiotic IR Type |
|
Spectral Type |
B3IIIe |
Magnitude range (V) |
|
Outbursts |
No |
|
|
Identifiers
Position
Right ascension (°) |
83.377143 ± 0.347400 |
Parallax (mas) |
– |
Reddening E(B-V) (mag) |
0.975 ± 0.231 |
Declination (°) |
-69.8741645 ± 0.382500 |
Distance (kpc) |
49.97 ± 0.19 |
|
|
Galactic longitude (°) |
280.436801 ± 0.382500 |
Proper motion in α (mas/yr) |
3.857 ± 0.683 |
|
|
Galactic latitude (°) |
-32.023949 ± 0.347400 |
Proper motion in δ (mas/yr) |
0.655 ± 1.028 |
|
|
Observations
U (mag) |
|
X-Ray |
|
Flickering |
|
B (mag) |
16.04 |
X-Ray type |
|
Outbursts |
No |
V (mag) |
16.61 |
IUE |
No |
Type |
|
R (mag) |
16.15 |
IRAS flux at 12 μm (Jy) |
|
IPmax (eV) |
|
I (mag) |
16.47 |
IRAS flux at 25 μm (Jy) |
|
OVI lines |
|
G (mag) |
19.36 |
IRAS flux at 60 μm (Jy) |
|
|
|
J (mag) |
14.68 |
IRAS flux at 100 μm (Jy) |
|
|
|
H (mag) |
12.94 |
WISE W1 (mag) |
10.87 |
|
|
K (mag) |
12.06 |
WISE W2 (mag) |
10.70 |
|
|
L (mag) |
|
WISE W3 (mag) |
6.89 |
|
|
|
|
WISE W4 (mag) |
3.72 |
|
|
|
|
Radio |
|
|
|
|
|
Radio flux (mJy) |
|
|
|
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 |
|
Ephemeris type |
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|
|
Mass ratio |
|
Ephemeris T0 (JD) |
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|
|
Cool component
Spectral type |
B3III[e] |
Mass (M⊙) |
|
Pulsation |
|
Eff. temperature (K) |
|
Radius (R⊙) |
|
Type |
|
IR type |
|
Luminosity (L⊙) |
|
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) |
|
Radius (R⊙) |
|
Accretion disk |
|
Lower limit (K) |
|
Luminosity (L⊙) |
|
|
|
Upper limit (K) |
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Links
SIMBAD CDS Portal
Notes
Reid & Parker (2006) classified the star as a possible symbiotic star. Later, Reid & Parker (2012) classified the star as B giant. Miszalski et al. (2011) classified the object as HII region and according to their analysis, VMC and SAGE data are consistent with the dusty environment. Finally, Reid (2014) classified the object as an emission line star.
References
- Miszalski, B., Napiwotzki, R., Cioni, M. R. L., et al., 2011, A&A, 531, A157, 2011A&A…531A.157M
- Reid, W. A., Parker, Q. A., 2006, MNRAS, 373, 521, 2006MNRAS.373..521R
- Reid, W. A., Parker, Q. A., 2012, MNRAS, 425, 355, 2012MNRAS.425..355R
- Reid, W. A., 2014, MNRAS, 438, 2642, 2014MNRAS.438.2642R
Last updated: May 11, 2019 @ 10:04 am