Accretion processes in star formation
- Lee Hartmann.
- 2nd ed.
- Cambridge ; New York : Cambridge University Press, 2009.
- Physical description
- xiv, 332 p. : ill. ; 25 cm.
- Cambridge astrophysics series ; 47.
- Hartmann, Lee, 1950-
- Includes bibliographical references (p. 306-327) and index.
- 1. Overview-- 2. Beginnings: molecular clouds-- 3. Initial conditions for protostellar collapse-- 4. Protostellar cloud collapse-- 5. Protostellar collapse: observations vs theory-- 6. Binaries, clusters, and the IMF-- 7. Disk accretion-- 8. The disks of pre-main sequence stars-- 9. The FU Orionis objects-- 10. Disk winds, jets, and magnetospheric accretion-- 11. Disk accretion and early stellar evolution-- 12. Disk evolution and planet formation-- Appendixes-- References-- Index.
- (source: Nielsen Book Data)
- Publisher's Summary
- 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 the book. The author brings together current observations, rigorous treatments of the relevant astrophysics, and 150 illustrations, to clarify the sequence of events in star and planet formation. It is a comprehensive account of the underlying physical processes of accretion for graduate students and researchers.
(source: Nielsen Book Data)
- Publication date
- Cambridge astrophysics series ; 47
- Previous ed.: 1998.
- 9780521531993 (pbk.)
- 0521531993 (pbk.)
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