A 2003 graduate text describing the theory astronomers need for studying globular star clusters.
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Douglas Heggie is Professor of Mathematical Astronomy at the University of Edinburgh, Scotland.
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Anbieter: Majestic Books, Hounslow, Vereinigtes Königreich
Zustand: New. pp. 372 69:B&W 6.69 x 9.61 in or 244 x 170 mm (Pinched Crown) Case Laminate on White w/Gloss Lam. Artikel-Nr. 7392921
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Anbieter: Romtrade Corp., STERLING HEIGHTS, MI, USA
Zustand: New. This is a Brand-new US Edition. This Item may be shipped from US or any other country as we have multiple locations worldwide. Artikel-Nr. ABBB-143557
Anbieter: Ria Christie Collections, Uxbridge, Vereinigtes Königreich
Zustand: New. In. Artikel-Nr. ria9780521773034_new
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Anbieter: Kennys Bookstore, Olney, MD, USA
Zustand: New. A 2003 graduate text describing the theory astronomers need for studying globular star clusters. Num Pages: 372 pages, 85 b/w illus. 5 tables 136 exercises. BIC Classification: PGM; PHVB. Category: (P) Professional & Vocational. Dimension: 177 x 251 x 22. Weight in Grams: 922. . 2003. Illustrated. hardcover. . . . . Books ship from the US and Ireland. Artikel-Nr. V9780521773034
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Anbieter: AHA-BUCH GmbH, Einbeck, Deutschland
Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - The globular star clusters of the Milky Way contain hundreds of thousands of stars held together by gravitational interactions, and date from the time when the Milky Way was forming. This 2003 text describes the theory astronomers need for studying globular star clusters. The gravitational million-body problem is an idealised model for understanding the dynamics of a cluster with a million stars. After introducing the million-body problem from various view-points, the book systematically develops the tools needed for studying the million-body problems in nature, and introduces the most important theoretical models. Including a comprehensive treatment of few-body interactions, and developing an intuitive but quantitative understanding of the three-body problem, the book introduces numerical methods, relevant software, and current problems. Suitable for graduate students and researchers in astrophysics and astronomy, this text also has important applications in the fields of theoretical physics, computational science and mathematics. Artikel-Nr. 9780521773034
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