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Spectroscopy of Stellar Coronal Sources with the Medium Energy Experiment on EXOSAT

Published online by Cambridge University Press:  12 April 2016

R. Pallavicini ,
L. Pasquini ,
J.H.M.M. Schmitt  and
G. Tagliaferri
R. Pallavicini
Affiliation:
Arcetri Astrophysical Observatory, Florence, Italy
L. Pasquini
Affiliation:
Max-Planck-lnstitut fur Extraterrestrische Physik, Garching, Germany
J.H.M.M. Schmitt
Affiliation:
Max-Planck-lnstitut fur Extraterrestrische Physik, Garching, Germany
G. Tagliaferri
Affiliation:
ESTEC, EXOSAT Observatory, Noordwijk, The Netherlands

Abstract

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We summarize some of the results obtained by spectral analysis of EXOSAT ME observations of stellar coronal sources. We focus on time-resolved spectroscopy of stellar flares and on the determination of the temperature structure of quiescent RS CVn binaries

Type
3. Stellar Coronae
Information
International Astronomical Union Colloquium , Volume 115: High Resolution X-ray Spectroscopy of Cosmic Plasmas , 1990 , pp. 122 - 125
Copyright
Copyright © Cambridge University Press 1990

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