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Stellar Coronae
Published online by Cambridge University Press: 13 May 2016
Abstract
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
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- Copyright © Astronomical Society of the Pacific 2001