CONFIRMED LMC
Equatorial coordinates
α = 86.331387 ± 0.084740 | 05 45 19.569000
δ = -71.268560 ± 0.102012 |-71 16 06.720000 |
|
Constellation |
Mensa |
Symbiotic IR Type |
D’ |
Spectral Type |
|
Magnitude range (V) |
|
Outbursts |
Yes? |
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|
Identifiers
Position
Right ascension (°) |
86.331387 ± 0.084740 |
Parallax (mas) |
– |
Reddening E(B-V) (mag) |
0.232 ± 0.022 |
Declination (°) |
-71.268560 ± 0.102012 |
Distance (kpc) |
49.97 ± 0.19 |
|
|
Galactic longitude (°) |
281.912253 ± 0.102012 |
Proper motion in α (mas/yr) |
2.243883 ± 0.179659 |
|
|
Galactic latitude (°) |
-30.873125 ± 0.084740 |
Proper motion in δ (mas/yr) |
0.751641 ± 0.205047 |
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|
Observations
U (mag) |
16.86 |
X-Ray |
No |
Flickering |
|
B (mag) |
17.41 |
X-Ray type |
|
Outbursts |
Yes? |
V (mag) |
17.06 |
IUE |
Yes |
Type |
|
R (mag) |
15.69 |
IRAS flux at 12 μm (Jy) |
<0.1258 |
IPmax (eV) |
114.0 |
I (mag) |
16.83 |
IRAS flux at 25 μm (Jy) |
0.1151 |
OVI lines |
Yes |
G (mag) |
17.17 |
IRAS flux at 60 μm (Jy) |
<0.2748 |
|
|
J (mag) |
15.92 |
IRAS flux at 100 μm (Jy) |
<2.189 |
|
|
H (mag) |
15.23 |
WISE W1 (mag) |
11.31 |
|
|
K (mag) |
13.01 |
WISE W2 (mag) |
9.79 |
|
|
L (mag) |
|
WISE W3 (mag) |
6.96 |
|
|
|
|
WISE W4 (mag) |
4.98 |
|
|
|
|
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) |
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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 |
|
Mass (M⊙) |
|
Pulsation |
|
Eff. temperature (K) |
4276 |
Radius (R⊙) |
|
Type |
|
IR type |
D’ |
Luminosity (L⊙) |
|
Pulsation period (days) |
|
Metallicity [Fe/H] |
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|
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Ephemeris type |
|
|
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|
|
Ephemeris T0 (JD) |
|
Hot component
Type/Spectra |
|
Mass (M⊙) |
|
Spin period (min) |
|
Eff. temperature (K) |
130000 ± 30000 |
Radius (R⊙) |
0.092 |
Accretion disk |
|
Lower limit (K) |
|
Luminosity (L⊙) |
2400 ± 1200 |
|
|
Upper limit (K) |
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Links
SIMBAD CDS Portal VSX
Notes
Usually classified as a SySt, but no direct evidence exists in the optical to confirm the presence of the giant component. Angeloni et al. (2011) discovered a giant, 14 parsecs long, highly collimated jet from the star. For at least two decades, Sanduleak’s star has been monotonically fading at an apparently constant rate of ∼0.03 mag/yr in all bands (Angeloni et al., 2014).
References
- Akras, S., Guzman-Ramirez, L., Leal-Ferreira, M. L., et al., 2019, ApJS, 240, 21, 2019ApJS..240…21A
- Allen, D. A., 1980, Astrophysical Letters, 20, 131, 1980ApL….20..131A
- Angeloni, R., Di Mille, F., Bland-Hawthorn, J., et al., 2011, ApJ, 743, L8, 2011ApJ…743L…8A
- Angeloni, R., Ferreira Lopes, C. E., Masetti, N., et al., 2014, MNRAS, 438, 35, 2014MNRAS.438…35A
- Heo, J. E., Angeloni, R., Di Mille, F., et al., 2016, ApJ, 833, 286, 2016ApJ…833..286H
- Muerset, U., Schild, H., Vogel, M., 1996, A&A, 307, 516, 1996A&A…307..516M
- Muerset, U., Wolff, B., Jordan, S., 1997, A&A, 319, 201, 1997A&A…319..201M
- Phillips, J. P., 2007, MNRAS, 376, 1120, 2007MNRAS.376.1120
- Sanduleak, N., 1977, Information Bulletin on Variable Stars, 1304, 1, 1977IBVS.1304….1S
Last updated: May 2, 2019 @ 11:25 am