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Title:
The asymmetric light curves of the GSC 2764 1417 (And), GSC 3355 0394 (Per) and GSC 2537 0520 (Psc)
Authors:
Samec, Ronald G.; Figg, Evan R.; Melton, Reid; Labadorf, Christa M.; Miller, Jess; McKenzie, Robert; Faulkner, Danny R.; Van Hamme, Walter
Affiliation:
AA(Astronomy program, Physics Department, Bob Jones University, Greenville, SC, USA ), AB(Astronomy program, Physics Department, Bob Jones University, Greenville, SC, USA ), AC(Astronomy program, Physics Department, Bob Jones University, Greenville, SC, USA ), AD(Astronomy program, Physics Department, Bob Jones University, Greenville, SC, USA ), AE(Astronomy program, Physics Department, Bob Jones University, Greenville, SC, USA ), AF(Astronomy program, Physics Department, Bob Jones University, Greenville, SC, USA ), AG(University of South Carolina, Lancaster, USA ), AH(Florida International University, Florida, USA )
Publication:
Solar and Stellar Variability: Impact on Earth and Planets, Proceedings of the International Astronomical Union, IAU Symposium, Volume 264, p. 75-77
Publication Date:
02/2010
Origin:
CUP
Keywords:
binaries: close, stars: activity, spots, mass loss, winds, outflows, techniques: photometric
DOI:
10.1017/S1743921309992407
Bibliographic Code:
2010IAUS..264...75S

Abstract

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).

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Database: Astronomy
Physics
arXiv e-prints