dynamical evolution star clusters (38 résultats)

HardBack. Etat : 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.

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hardcover. Etat : New. In shrink wrap. Looks like an interesting title!

Etat : New. pp. 432.

Taschenbuch. Etat : 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. Etat : 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. Etat : 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. Etat : 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.

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Hardcover. Etat : Like New. LIKE NEW. SHIPS FROM MULTIPLE LOCATIONS. book.

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Taschenbuch. Etat : 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.

Buch. Etat : 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.

PAP. Etat : New. New Book. Delivered from our UK warehouse in 4 to 14 business days. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000.

HRD. Etat : New. New Book. Delivered from our UK warehouse in 4 to 14 business days. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000.

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Paperback. Etat : new. Paperback. "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. This item is printed on demand. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability.

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Hardcover. Etat : new. Hardcover. "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. This item is printed on demand. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability.

LeatherBound. Etat : New. BOOKS ARE EXEMPT FROM IMPORT DUTIES AND TARIFFS; NO EXTRA CHARGES APPLY. LeatherBound edition. Condition: New. Reprinted from 1910 edition. Leather Binding on Spine and Corners with Golden leaf printing on spine. Bound in genuine leather with Satin ribbon page markers and Spine with raised gilt bands. A perfect gift for your loved ones. Pages: 887 NO changes have been made to the original text. This is NOT a retyped or an ocr'd reprint. Illustrations, Index, if any, are included in black and white. Each page is checked manually before printing. As this print on demand book is reprinted from a very old book, there could be some missing or flawed pages, but we always try to make the book as complete as possible. Fold-outs, if any, are not part of the book. If the original book was published in multiple volumes then this reprint is of only one volume, not the whole set. Sewing binding for longer life, where the book block is actually sewn (smythe sewn/section sewn) with thread before binding which results in a more durable type of binding. Pages: 887.

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Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -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. 428 pp. Englisch.