Please use this identifier to cite or link to this item:
Title: Circumbinary planet study around NSVS 14256825
Authors: P. Sappankum
S. Komonjinda
S. Awiphan
R. Rattanamala
V. S. Dhillon
T. R. Marsh
S. Suphapolthaworn
Keywords: Physics and Astronomy
Issue Date: 16-Dec-2019
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.
ISSN: 17426596
Appears in Collections:CMUL: Journal Articles

Files in This Item:
There are no files associated with this item.

Items in CMUIR are protected by copyright, with all rights reserved, unless otherwise indicated.