Circumbinary planet study around NSVS 14256825
© Published under licence by IOP Publishing Ltd. The period variability of (O-C) diagram of an eclipsing binary, NSVS 14256825, which is composed of a hot subdwarf type OB star (sdOB) and a main-sequence low-mass type M star (dM) in close orbit with period P=0.110374 days, previously showed sinusoid...
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| Main Authors: | , , , , , , |
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| 格式: | Conference Proceeding |
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2020
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| 主題: | |
| 在線閱讀: | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85077810071&origin=inward http://cmuir.cmu.ac.th/jspui/handle/6653943832/68080 |
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| 機構: | Chiang Mai University |