Cool stars, stellar systems, and the sun : proceedings of the Fifth Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, held in Boulder, Colorado, July 7-11, 1987 /

Cool stars, stellar systems, and the sun : proceedings of the Fifth Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, held in Boulder, Colorado, July 7-11, 1987 /

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Bibliographic Details
Meeting name:	Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (5th : 1987 : Boulder, Colo.)
Imprint:	Berlin ; New York : Springer-Verlag, ©1987.
Description:	1 online resource (xiii, 537 pages) : illustrations.
Language:	English
Series:	Lecture notes in physics, 0075-8450 ; 291 Lecture notes in physics ; 291.
Subject:	Stars -- Congresses. Cool stars -- Congresses. Cool stars. Stars. Sun -- Congresses. Sun. Conference papers and proceedings.
Format:	E-Resource Book
URL for this record:	http://pi.lib.uchicago.edu/1001/cat/bib/11067285

Hidden Bibliographic Details
Other authors / contributors:	Linsky, J. L. (Jeffrey L.), 1941- Stencel, Robert E.
ISBN:	9783540480419 3540480412 9783540186533 0387186530 9780387186535
Notes:	Includes bibliographical references and index. Restrictions unspecified Electronic reproduction. [S.l.] : HathiTrust Digital Library, 2010. Master and use copy. Digital master created according to Benchmark for Faithful Digital Reproductions of Monographs and Serials, Version 1. Digital Library Federation, December 2002. http://purl.oclc.org/DLF/benchrepro0212 digitized 2010 HathiTrust Digital Library committed to preserve Print version record.
Summary:	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).
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