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Stellar Coronae

Published online by Cambridge University Press:  13 May 2016

J. H. M. M. Schmitt
J. H. M. M. Schmitt*
Affiliation:
Hamburger Sternwarte, 21029 Hamburg, Gojenbergsweg 112, Germany

Abstract

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The last two decades have seen the emergence of a new field in stellar astrophysics, the study of stellar coronae mostly in X-ray domain. With the advent of soft X-ray imagery X-ray emission was found from many thousands of solar-like stars. I will summarize the most important findings of X-ray surveys of late type stars and put the results in the context of the solar-stellar connection.

Type
Session V: Coronal Heating and Solar Wind Acceleration
Information
Symposium - International Astronomical Union , Volume 203: Recent Insights into the Physics of the Sun and Heliosphere: Highlights from Soho and Other Space Missions , 2001 , pp. 475 - 487
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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