Please use this identifier to cite or link to this item: http://cmuir.cmu.ac.th/jspui/handle/6653943832/68080
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dc.contributor.authorP. Sappankumen_US
dc.contributor.authorS. Komonjindaen_US
dc.contributor.authorS. Awiphanen_US
dc.contributor.authorR. Rattanamalaen_US
dc.contributor.authorV. S. Dhillonen_US
dc.contributor.authorT. R. Marshen_US
dc.contributor.authorS. Suphapolthawornen_US
dc.date.accessioned2020-04-02T15:18:14Z-
dc.date.available2020-04-02T15:18:14Z-
dc.date.issued2019-12-16en_US
dc.identifier.issn17426596en_US
dc.identifier.issn17426588en_US
dc.identifier.other2-s2.0-85077810071en_US
dc.identifier.other10.1088/1742-6596/1380/1/012095en_US
dc.identifier.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85077810071&origin=inwarden_US
dc.identifier.urihttp://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.subjectPhysics and Astronomyen_US
dc.titleCircumbinary planet study around NSVS 14256825en_US
dc.typeConference Proceedingen_US
article.title.sourcetitleJournal of Physics: Conference Seriesen_US
article.volume1380en_US
article.stream.affiliationsNakhonratchasima Rajabhat Universityen_US
article.stream.affiliationsThe University of Warwicken_US
article.stream.affiliationsHokkaido Universityen_US
article.stream.affiliationsUniversity of Sheffielden_US
article.stream.affiliationsChiang Mai Universityen_US
article.stream.affiliationsNational Astronomical Research Institute of Thailanden_US
Appears in Collections:CMUL: Journal Articles

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