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Physics of star formation in galaxies

Author: F Palla; Hans Zinnecker; André Maeder; G Meynet
Publisher: Berlin ; New York : Springer, ©2002.
Series: Saas-Fee advanced course ... lecture notes, 1999.
Edition/Format:   eBook : Document : EnglishView all editions and formats
Summary:
The book begins with a historical introduction, "Star Formation: The Early History", that presents new material of interest for students and historians of science. This is followed by two long articles on "Pre-Main-Sequence Evolution of Stars and Young Clusters" and "Observations of Young Stellar Objects". These articles on the fascinating problem of star formation from interstellar matter give a thorough overview  Read more...
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Genre/Form: Electronic books
Additional Physical Format: Print version:
Palla, F. (Francesco).
Physics of star formation in galaxies.
Berlin ; New York : Springer, ©2002
(DLC) 2002022168
Material Type: Document, Internet resource
Document Type: Internet Resource, Computer File
All Authors / Contributors: F Palla; Hans Zinnecker; André Maeder; G Meynet
ISBN: 3540316337 9783540316336 1280624043 9781280624049
OCLC Number: 228372251
Description: 1 online resource (xii, 232 pages) : illustrations.
Contents: Historical Introduction. Star Formation: the Early History (G. Herbig) --
Pre-Main-Sequence Evolution of Stars and Young Clusters (F. Palla): I. Initial Conditions of Pre-Main-Sequence Evolution --
II. Pre-Main-Sequence Evolution --
III. Physical Processes in PMS Stars --
IV. PMS Evolution of Clusters and Associations --
Observations of Young Stellar Objects (YSO) (H. Zinnecker): I. Introduction --
II. Disks, Jets and Protostars --
III. Young Binaries --
IV. Low-Mass Stellar Content of Young Star Clusters and Associations --
Index.
Series Title: Saas-Fee advanced course ... lecture notes, 1999.
Responsibility: F. Palla, H. Zinnecker ; edited by A. Maeder and G. Meynet ; with an introduction by George Herbig.

Abstract:

The book begins with a historical introduction, "Star Formation: The Early History", that presents new material of interest for students and historians of science. This is followed by two long  Read more...

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