Circumbinary planet study around NSVS 14256825

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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Bibliographic Details
Main Authors: P. Sappankum, S. Komonjinda, S. Awiphan, R. Rattanamala, V. S. Dhillon, T. R. Marsh, S. Suphapolthaworn
Format: Conference Proceeding
Published: 2020
Subjects:
Physics and Astronomy
Online Access: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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Institution: Chiang Mai University

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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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