Circumbinary planet study around NSVS 14256825

• المؤلفون الرئيسيون: P. Sappankum, S. Komonjinda, S. Awiphan, R. Rattanamala, V. S. Dhillon, T. R. Marsh, S. Suphapolthaworn
• التنسيق: وقائع المؤتمر
• منشور في: 2020
• الموضوعات: Physics and Astronomy
• الوصول للمادة أونلاين: https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85077810071&origin=inward; http://cmuir.cmu.ac.th/jspui/handle/6653943832/68080
• المؤسسة: Chiang Mai University

© 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...