Cool Stars, Stellar Systems and the Sun

Cool Stars, Stellar Systems and the Sun

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Recent research on the solar-stellar system has been triggered by a host of recent observational data, in particular from space based observations. For this conference the major topics selected centered on new measurement capabilities (magnetic fields and infrared, with specific emphasis on the new IRAS results), important classes of stars (F stars, M dwarfs and giants, and pre-main sequence stars), and interesting unanswered questions (the nature of nonthermal phenomena, heating processes, angular momentum evolution, and the existence and cause of the corona/wind dividing line). Each section is opened by two or more invited lectures aimed at a wide audience, including graduate students, and continues with some research papers. The proceedings also record the two general discussions on the role of magnetic fields in cool star atmospheres and the role of monitoring programs for studies of cool stars (see also Lecture Notes in Physics Vol. 292).Mariska: My calculations indicate that one must go to smaller and smaller loops. ... Mariska: Small hot loops which are conduction-dominated will have the temperature and the flow structure I have ... The velocity peak at 105K is due to a combination of the actual velocity versus temperature profile of the loop, and the anbsp;...

Title:Cool Stars, Stellar Systems and the Sun
Author:Jeffrey L. Linsky, Robert E. Stencel
Publisher: - 1987


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