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An Update on X-Ray Emission from Stars
Published online by Cambridge University Press: 14 August 2015
Abstract
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.
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- Joint Commission Meeting
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- Copyright © Kluwer 1989