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An Update on X-Ray Emission from Stars

Published online by Cambridge University Press:  14 August 2015

R. Rosner
R. Rosner*
Affiliation:
Enrico Fermi Institute and Dept. of Astronomy and Astrophysics, The University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637

Abstract

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With the closing of the Einstein and EXOSAT eras, the characteristics of stellar x-ray emission are now fairly well understood. In this very brief review, I will focus on two specific topics central to the physics underlying stellar activity: the rotation-activity connection and the “decay” of activity at the low mass end of the main sequence.

Type
Joint Commission Meeting
Information
Highlights of Astronomy , Volume 8: Highlights of Astronomy. As presented at the XXth General Assembly of the IAU, 1988 , 1989 , pp. 521 - 524
Copyright
Copyright © Kluwer 1989

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