Photometry of Eclipsing Binary Stars in the Large and Small Magellanic Clouds
2004 ◽
Vol 191
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pp. 116-120
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AbstractThe light curves for three eclipsing binaries in the Magellanic Clouds have been obtained using CCD uVJIC photometry. One target in the LMC, MACHO*05:36:48.7−69:17:00, is an eccentric system, e = 0.20, with a period of 3.853534 ± 0.000005 d. Initial solutions indicate a primary component in the range Teff,1 = 20,000−35,000K and the secondary Teff,2 1000−2000K cooler than the primary, with inclinations ranging i = 84.2° − 86.0°. Two targets in the SMC, MOA J005018.4-723855 and MOA J005623.5−722123, have periods of 1.8399±0.0004 and 2.3199 ± 0.0003 days respectively. Both have circular orbits with the former being a semi-detached system.
2004 ◽
Vol 193
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pp. 407-410
2016 ◽
Vol 151
(4)
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pp. 101
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2006 ◽
Vol 2
(S239)
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pp. 157-159
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2020 ◽
Vol 496
(3)
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pp. 2605-2612
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2008 ◽
Vol 4
(S258)
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pp. 161-170
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2020 ◽
Vol 497
(3)
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pp. 2899-2909
2003 ◽
Vol 31
(2)
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pp. 393-398
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Keyword(s):
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