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The asymmetric light curves of the GSC 2764 1417 (And), GSC 3355 0394 (Per) and GSC 2537 0520 (Psc)

Published online by Cambridge University Press:  26 February 2010

Ronald G. Samec ,
Evan R. Figg ,
Reid Melton ,
Christa M. Labadorf ,
Jess Miller ,
Robert McKenzie ,
Danny R. Faulkner  and
Walter Van Hamme
Ronald G. Samec
Affiliation:
Astronomy program, Physics Department, Bob Jones University, Greenville, SC, USA email: [email protected]
Evan R. Figg
Affiliation:
Astronomy program, Physics Department, Bob Jones University, Greenville, SC, USA email: [email protected]
Reid Melton
Affiliation:
Astronomy program, Physics Department, Bob Jones University, Greenville, SC, USA email: [email protected]
Christa M. Labadorf
Affiliation:
Astronomy program, Physics Department, Bob Jones University, Greenville, SC, USA email: [email protected]
Jess Miller
Affiliation:
Astronomy program, Physics Department, Bob Jones University, Greenville, SC, USA email: [email protected]
Robert McKenzie
Affiliation:
Astronomy program, Physics Department, Bob Jones University, Greenville, SC, USA email: [email protected]
Danny R. Faulkner
Affiliation:
University of South Carolina, Lancaster, USA email: [email protected]
Walter Van Hamme
Affiliation:
Florida International University, Florida, USA email: [email protected]
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Abstract

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Solar-type variability is enhanced in short period close binaries with increased dynamo driven activity. This activity is studied in our analysis of recent light curves taken of the newly discovered eclipsing binaries GSC 2764 1417 (And), GSC 3355 0394 (Per) and GSC 2537 0775 (CVn).

Keywords

binaries: closestars: activityspotsmass losswindsoutflowstechniques: photometric
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S264: Solar and Stellar Variability: Impact on Earth and Planets , August 2009 , pp. 75 - 77
Copyright
Copyright © International Astronomical Union 2010

References

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