Searching for planets around eclipsing binary stars using timing method: NSVS 14256825
2017 ◽
Vol 12
(S330)
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pp. 405-406
AbstractWe present four new mid eclipse times and an updated O-C diagram of the short period eclipsing binary NSVS14256825. The new data follow the (O-C) trend and its model proposed in Nasiroglu et al. (2017). The (O-C) diagram shows quasi-periodic variations that can be explained with the presence of a brown-dwarf in a quasi-circular circumbinary orbit.
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2012 ◽
Vol 124
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pp. 535-544
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2006 ◽
Vol 2
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pp. 157-159
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2005 ◽
Vol 362
(3)
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pp. 1006-1014
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2020 ◽
Vol 496
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pp. 2605-2612
2020 ◽
Vol 497
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pp. L19-L23
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2016 ◽
Vol 152
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pp. 180
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