Abstract
Within the last few years there have been important advances in our understanding of the chromospheres, coronae, and winds of late-type stars. This progress has been the result of ultraviolet and X-ray observations obtained from space with theInternational Ultraviolet Explorer andEinstein satellites. In addition, ground-based astronomy has contributed much to synoptic studies of stellar activity. In this review I summarize some of the major recent developments in this field.
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Simon, T. Stellar chromospheres, coronae, and winds (invited review). Astrophys Space Sci 118, 209–222 (1986). https://doi.org/10.1007/BF00651128
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DOI: https://doi.org/10.1007/BF00651128