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Lightcurve studies and magnetic activities of several eclipsing binaries

Published online by Cambridge University Press:  09 September 2016

Xianming L. Han ,
Liyun Zhang ,
Qingfeng Pi  and
Daimei Wang
Xianming L. Han
Affiliation:
Department of Physics, College of Science, Guizhou University and NAOC-GZU-Sponsored Center for Astronomy, Guizhou University, Guiyang 550025, P.R. China Dept. of Physics and Astronomy, Butler University, Indianapolis, IN 46208, USA email: xhan@butler.edu
Liyun Zhang
Affiliation:
Department of Physics, College of Science, Guizhou University and NAOC-GZU-Sponsored Center for Astronomy, Guizhou University, Guiyang 550025, P.R. China
Qingfeng Pi
Affiliation:
Department of Physics, College of Science, Guizhou University and NAOC-GZU-Sponsored Center for Astronomy, Guizhou University, Guiyang 550025, P.R. China
Daimei Wang
Affiliation:
Department of Physics, College of Science, Guizhou University and NAOC-GZU-Sponsored Center for Astronomy, Guizhou University, Guiyang 550025, P.R. China
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Abstract

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Late-type stars with thick convective zones and rapid rotations exhibit magnetic activity phenomena, such as starspots, plages, and flares. However, in many such kinds of eclipsing binaries, the details of the active phenomena are not well understood. In order to improve our understanding of stellar magnetic activities, we are carrying out an extensive study of the magnetic activities of eclipsing binaries by multi-color CCD photometry using several telescopes (SARA 90cm at KPNO, and NAOC 85cm and 60 cm telescopes at Xinglong). In this paper, we will present our preliminary results with revised orbital parameters, starspot parameters, and stellar flare events on DV Psc and BX Tri.

Keywords

stars: individual (DV Psc, BX Tri)stars: flarestars: activitybinaries: eclipsing
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S320: Solar and Stellar Flares and their Effects on Planets , August 2015 , pp. 321 - 323
Copyright
Copyright © International Astronomical Union 2016 

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