dynamical evolution star clusters (11 Ergebnisse)

HardBack. Zustand: Good. xviii, 406pp. ill. Good clean copy. Confrontation of Theory and Observations -proceedings of the 174th symposium of the International Astronomical Union, held in Tokyo, Japan, August 22-25, 1995.

Zustand: New. In.

Zustand: New. In.

Taschenbuch. Zustand: Neu. Dynamical Evolution of Star Clusters - Confrontation of Theory and Observations | Junichiro Makino (u. a.) | Taschenbuch | xviii | Englisch | 1996 | Springer | EAN 9780792340706 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.

Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - This volume reviews recent progress in the study of dynamics of star clusters. The meeting focused on the enormous progress of both the observation and the theoretical modeling of star clusters. New results from the refurbished Hubble Space Telescope (HST) include the mass function down to the hydrogen burning limits, white dwarf sequence, and central density profiles of `post-collapse' clusters by star counts. On the theoretical side, this symposium saw the first direct evidence of gravothermal oscillation through N-body simulation, which was made possible by GRAPE-4, the dedicated special-purpose computer for N-body simulation. Numerical techniques to combine stellar evolution and dynamical evolution of the cluster were presented. The book will be of primary interest to astrophysicists.

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - This volume reviews recent progress in the study of dynamics of star clusters. The meeting focused on the enormous progress of both the observation and the theoretical modeling of star clusters. New results from the refurbished Hubble Space Telescope (HST) include the mass function down to the hydrogen burning limits, white dwarf sequence, and central density profiles of `post-collapse' clusters by star counts. On the theoretical side, this symposium saw the first direct evidence of gravothermal oscillation through N-body simulation, which was made possible by GRAPE-4, the dedicated special-purpose computer for N-body simulation. Numerical techniques to combine stellar evolution and dynamical evolution of the cluster were presented. The book will be of primary interest to astrophysicists.

Couverture souple. Zustand: bon. R260269820: 1996. In-8. Broché. Très bon état, Couv. convenable, Dos satisfaisant, Intérieur frais. 406 pages augmentées de quelques figures en noir et blanc dans texte. . . . Classification Dewey : 420-Langue anglaise. Anglo-saxon.

Zustand: New. Reviews progress in the study of dynamics of star clusters. This title presents numerical techniques to combine stellar evolution and dynamical evolution of the cluster. It is intended for astrophysicists. Editor(s): Hut, Piet. Series: International Astronomical Union Symposia (Closed). Num Pages: 424 pages, biography. BIC Classification: PGM; PHD. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly; (UU) Undergraduate. Dimension: 234 x 156 x 22. Weight in Grams: 597. . 1996. Paperback. . . . . Books ship from the US and Ireland.

Zustand: New. Reviews progress in the study of dynamics of star clusters. This book is of primary interest to astrophysicists. Editor(s): Hut, Piet; Makino, Junichiro. Series: International Astronomical Union Symposia (Closed). Num Pages: 424 pages, biography. BIC Classification: PGM; PHD. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly; (UU) Undergraduate. Dimension: 235 x 155 x 23. Weight in Grams: 779. . 1996. Hardback. . . . . Books ship from the US and Ireland.

Taschenbuch. Zustand: Neu. Neuware - 'The Capture Theory Of Cosmical Evolution' presents Thomas Jefferson Jackson See's comprehensive exploration of the universe's development, grounded in dynamical principles and observational evidence. This meticulously researched work delves into the formation and evolution of celestial bodies, drawing insights from spiral nebulae, our planetary system, double and multiple stars, star clusters, and the Milky Way's star-clouds. See's detailed analysis offers a unique perspective on the cosmos, challenging conventional theories of his time. By integrating rigorous scientific methodologies with extensive astronomical observations, this book provides a foundational understanding of the forces shaping the universe. It remains a valuable resource for students, researchers, and anyone fascinated by the intricacies of space and the processes governing its evolution.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.

Buch. Zustand: Neu. Neuware - 'The Capture Theory Of Cosmical Evolution' presents Thomas Jefferson Jackson See's comprehensive exploration of the universe's development, grounded in dynamical principles and observational evidence. This meticulously researched work delves into the formation and evolution of celestial bodies, drawing insights from spiral nebulae, our planetary system, double and multiple stars, star clusters, and the Milky Way's star-clouds.