Since it was first published in 1987, Galactic Dynamics has become the most widely used advanced textbook on the structure and dynamics of galaxies and one of the most cited references in astrophysics. Now, in this extensively revised and updated edition, James Binney and Scott Tremaine describe the dramatic recent advances in this subject, making Galactic Dynamics the most authoritative introduction to galactic astrophysics available to advanced undergraduate students, graduate students, and researchers.
Every part of the book has been thoroughly overhauled, and many sections have been completely rewritten. Many new topics are covered, including N-body simulation methods, black holes in stellar systems, linear stability and response theory, and galaxy formation in the cosmological context. Binney and Tremaine, two of the world's leading astrophysicists, use the tools of theoretical physics to describe how galaxies and other stellar systems work, succinctly and lucidly explaining theoretical principles and their applications to observational phenomena. They provide readers with an understanding of stellar dynamics at the level needed to reach the frontiers of the subject. This new edition of the classic text is the definitive introduction to the field. ?Les informations fournies dans la section « Synopsis » peuvent faire référence à une autre édition de ce titre.
James Binney is professor of physics at the University of Oxford. His books include Galactic Astronomy. Scott Tremaine is the Richard Black Professor of Astrophysics at the Institute for Advanced Study and a member of the National Academy of Sciences. Both are fellows of the Royal Society.
Les informations fournies dans la section « A propos du livre » peuvent faire référence à une autre édition de ce titre.
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Etat : New. 2008. Second. Paperback. Offers an introduction to galactic astrophysics to advanced undergraduate students, graduate students, and researchers. This book covers topics including N-body simulation methods, black holes in stellar systems, linear stability and response theory, and galaxy formation in the cosmological context. Series: Princeton Series in Astrophysics. Num Pages: 904 pages, 16 color illus. 205 halftones. BIC Classification: PHVB. Category: (P) Professional & Vocational; (U) Tertiary Education (US: College). Dimension: 232 x 156 x 41. Weight in Grams: 1276. . . . . . N° de réf. du vendeur V9780691130279
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