Giants of Eclipse: The ? Aurigae Stars and Other Binary Systems, Thomas B. Ake; Elizabeth Griffin
Автор: Ramon Lopez-Pena; Riccardo Capovilla; Ricardo Garc Название: Complex Systems and Binary Networks ISBN: 3662140578 ISBN-13(EAN): 9783662140574 Издательство: Springer Рейтинг: Цена: 15672.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: The five contributions describe some key mathematical concepts involved in the study of complex systems and non-perturbative problems. This pedagogically written text can be used as an introduction to the fundamental ideas behind complex systems theory.
Автор: Eggleton Название: Evolutionary Processes in Binary and Multiple Stars ISBN: 1107403421 ISBN-13(EAN): 9781107403420 Издательство: Cambridge Academ Рейтинг: Цена: 10611.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: This 2006 volume discusses the statistics of binary stars; the evolution of single stars; and several of the most important kinds of interaction between two (and even three or more) stars. A series of mathematical appendices gives a concise but full account of the mathematics of these processes.
Автор: Nader Haghighipour Название: Planets in Binary Star Systems ISBN: 9400732422 ISBN-13(EAN): 9789400732421 Издательство: Springer Рейтинг: Цена: 26120.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: The discovery of extrasolar planets has impacted on our understanding of planetary systems. This volume collates research into planets in binary and multistar systems and aims to familiarize readers with its associated theoretical and observational challenges.
Автор: E.F. Milone Название: Light Curve Modeling of Eclipsing Binary Stars ISBN: 1461276497 ISBN-13(EAN): 9781461276494 Издательство: Springer Рейтинг: Цена: 15672.00 р. Наличие на складе: Есть у поставщика Поставка под заказ.
Описание: In the two decades since the development of the first eclipsing-binary modeling code, new analytic techniques and the availability of powerful, sometimes dedicated computing facilities have made possible vastly improved determinations of fundamental and even transient stellar parameters.
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