On Chromospheric Emission and Photometric Variability of Active Late-Type Stars

Strassmeier, K. G.

doi:10.1007/978-94-009-0679-2_38

K. G. Strassmeier^2,3

Part of the book series: NATO ASI Series ((ASIC,volume 319))

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Abstract

To pursue the study of solar phenomena in late-type stars, we have investigated chromospheric activity in 100 single and binary stars of spectral type F6 to M2 and luminosity class III, IV, and V. Attempts are made to “quantify” starspot activity and correlate it to chromospheric activity.

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Authors and Affiliations

Department of Physics and Astronomy, Vanderbilt University, Nashville, TN, 37235, USA
K. G. Strassmeier
Center of Excellence in Information Systems, Tennessee State University, Nashville, TN, 37209-1561, USA
K. G. Strassmeier

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K. G. Strassmeier
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Editors and Affiliations

Astronomy and Space Sciences Department, Ege University Science Faculty, Bornova, Izmir, Turkey
Cafer İbanoğlu

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Strassmeier, K.G. (1990). On Chromospheric Emission and Photometric Variability of Active Late-Type Stars. In: İbanoğlu, C. (eds) Active Close Binaries. NATO ASI Series, vol 319. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0679-2_38

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DOI: https://doi.org/10.1007/978-94-009-0679-2_38
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-6790-4
Online ISBN: 978-94-009-0679-2
eBook Packages: Springer Book Archive

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