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DC Field | Value | Language |
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dc.contributor.author | P. Sappankum | en_US |
dc.contributor.author | S. Komonjinda | en_US |
dc.contributor.author | S. Awiphan | en_US |
dc.contributor.author | R. Rattanamala | en_US |
dc.contributor.author | V. S. Dhillon | en_US |
dc.contributor.author | T. R. Marsh | en_US |
dc.contributor.author | S. Suphapolthaworn | en_US |
dc.date.accessioned | 2020-04-02T15:18:14Z | - |
dc.date.available | 2020-04-02T15:18:14Z | - |
dc.date.issued | 2019-12-16 | en_US |
dc.identifier.issn | 17426596 | en_US |
dc.identifier.issn | 17426588 | en_US |
dc.identifier.other | 2-s2.0-85077810071 | en_US |
dc.identifier.other | 10.1088/1742-6596/1380/1/012095 | en_US |
dc.identifier.uri | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85077810071&origin=inward | en_US |
dc.identifier.uri | http://cmuir.cmu.ac.th/jspui/handle/6653943832/68080 | - |
dc.description.abstract | © 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 sinusoidal signal cause by the light travel time effects. This signal can be caused by the presence of third bodies. We re-examined (O-C) diagram of the system. We combined eclipse timings from published data and the data taken from ULTRASPEC at 2.4 m at Thai National Telescope on November 2018. From the fitting model, the parameters of the third body in NSVS 14256825 system are obtained. | en_US |
dc.subject | Physics and Astronomy | en_US |
dc.title | Circumbinary planet study around NSVS 14256825 | en_US |
dc.type | Conference Proceeding | en_US |
article.title.sourcetitle | Journal of Physics: Conference Series | en_US |
article.volume | 1380 | en_US |
article.stream.affiliations | Nakhonratchasima Rajabhat University | en_US |
article.stream.affiliations | The University of Warwick | en_US |
article.stream.affiliations | Hokkaido University | en_US |
article.stream.affiliations | University of Sheffield | en_US |
article.stream.affiliations | Chiang Mai University | en_US |
article.stream.affiliations | National Astronomical Research Institute of Thailand | en_US |
Appears in Collections: | CMUL: Journal Articles |
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