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Lee Hartmann - Accretion Processes in Star Formation - 9780521531993 - V9780521531993
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Accretion Processes in Star Formation

€ 94.37
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Description for Accretion Processes in Star Formation paperback. A complete account of the underlying physical processes of accretion for graduate students and researchers. Series: Cambridge Astrophysics. Num Pages: 346 pages, 60 b/w illus. BIC Classification: PGC; PGM; PHVB. Category: (UP) Postgraduate, Research & Scholarly. Dimension: 244 x 174 x 17. Weight in Grams: 694.
Our understanding of the formation of stars and planetary systems has changed greatly since the first edition of this book was published. This new edition has been thoroughly updated, and now includes material on molecular clouds, binaries, star clusters and the stellar initial mass function (IMF), disk evolution and planet formation. This book provides a comprehensive picture of the formation of stars and planetary systems, from their beginnings in cold clouds of molecular gas to their emergence as new suns with planet-forming disks. At each stage gravity induces an inward accretion of mass, and this is a central theme for ... Read more

Product Details

Format
Paperback
Publication date
2008
Publisher
Cambridge University Press United Kingdom
Number of pages
346
Condition
New
Series
Cambridge Astrophysics
Number of Pages
346
Place of Publication
Cambridge, United Kingdom
ISBN
9780521531993
SKU
V9780521531993
Shipping Time
Usually ships in 7 to 11 working days
Ref
99-12

About Lee Hartmann
Lee Hartmann is currently Professor of Astronomy at the University of Michigan and a vice-president of the American Astronomical Society. He is an expert on star formation and protoplanetary disk evolution.

Reviews for Accretion Processes in Star Formation
"Readers with the background to appreciate the mathematical and astrophysical arguments the author presents will find this text a valuable review of current thinking on star formation and proto-stellar disk evolution." - The Meteorological Society

Goodreads reviews for Accretion Processes in Star Formation


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