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Observed photometric peculiarities of six eclipsing binaries with solar-type activity: I

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Abstract

From the observed light curves of six eclipsing binaries with solar-type activity and from the analysis of their period variations some problems in the interpretation of the observations came out:

Are these binaries similar to classical RS CVn stars?

Is the stellar surface spot coverage the unique interpretation of the observed light curves?

Are these systems really linked with W UMa's?

In a further study some models will be tempted to try to solve these problems.

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Authors and Affiliations

  1. Department of Physics, Naples University, Italy

    L. Milano & S. Mancuso

  2. Capodimonte Astronomical Observatory, Naples, Italy

    A. Vittone, A. D'Orsi & S. Marcozzi

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  1. L. Milano
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  2. S. Mancuso
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  3. A. Vittone
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  4. A. D'Orsi
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  5. S. Marcozzi
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Milano, L., Mancuso, S., Vittone, A. et al. Observed photometric peculiarities of six eclipsing binaries with solar-type activity: I. Astrophys Space Sci 124, 83–100 (1986). https://doi.org/10.1007/BF00649751

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  • DOI: https://doi.org/10.1007/BF00649751

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