Stars form surrounded by a circumstellar disk which is thought to be the cradle of planets. IAU Symposium 243 highlights the latest developments in understanding the structure and evolution of the star-disk interaction region in young stars, a critical component of our knowledge of star and planetary system formation processes. Discussions review the physical processes thought to be at work at the star-disk interface, confront the predictions of the latest numerical and analytical magnetohydrodynamic models of star-disk-jet systems with observations, and explore the consequences of these processes for stellar angular momentum evolution and inner disk structure. The most recent observational results, computer simulations and theoretical developments in this active field of research are included to provide a unique vision into this central aspect of the star and planet formation problem.
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Stars form surrounded by a circumstellar disk which is thought to be the cradle of planets. IAU Symposium 243 highlights the latest developments in understanding the structure and evolution of the star-disk interaction region in young stars, a critical component of our knowledge of star and planetary system formation processes. Discussions review the physical processes thought to be at work at the star-disk interface, confront the predictions of the latest numerical and analytical magnetohydrodynamic models of star-disk-jet systems with observations, and explore the consequences of these processes for stellar angular momentum evolution and inner disk structure. The most recent observational results, computer simulations and theoretical developments in this active field of research are included to provide a unique vision into this central aspect of the star and planet formation problem.
'All in all this was a pretty good collection of papers discussing our current understanding of star-disc interactions ...' The Observatory: A Review of Astronomy
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Etat : New. Reviews latest star-disk interaction region in young stars for graduate students and researchers. Editor(s): Appenzeller, Immo; Bouvier, Jerome. Series: Proceedings of the International Astronomical Union Symposia and Colloquia. Num Pages: 390 pages, 231 b/w illus. 6 tables. BIC Classification: PG. Category: (P) Professional & Vocational. Dimension: 247 x 174 x 23. Weight in Grams: 918. . 2008. hardcover. . . . . Books ship from the US and Ireland. N° de réf. du vendeur 9780521874656
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Etat : New. Reviews latest star-disk interaction region in young stars for graduate students and researchers. Editor(s): Appenzeller, Immo; Bouvier, Jerome. Series: Proceedings of the International Astronomical Union Symposia and Colloquia. Num Pages: 390 pages, 231 b/w illus. 6 tables. BIC Classification: PG. Category: (P) Professional & Vocational. Dimension: 247 x 174 x 23. Weight in Grams: 918. . 2008. hardcover. . . . . N° de réf. du vendeur 9780521874656
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Cartoné (tapa dura cartón). Etat : New. Etat de la jaquette : Nuevo. 01. Description Contents Resources Courses About the Authors. Stars form surrounded by a circumstellar disk which is thought to be the cradle of planets. IAU Symposium 243 highlights the latest developments in understanding the structure and evolution of the star-disk interaction region in young stars, a critical component of our knowledge of star and planetary system formation processes. Discussions review the physical processes thought to be at work at the star-disk interface, confront the predictions of the latest numerical and analytical magnetohydrodynamic models of star-disk-jet systems with observations, and explore the consequences of these processes for stellar angular momentum evolution and inner disk structure. The most recent observational results, computer simulations and theoretical developments in this active field of research are included to provide a unique vision into this central aspect of the star and planet formation problem. LIBRO. N° de réf. du vendeur 887812
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Hardcover. Etat : new. Hardcover. Stars form surrounded by a circumstellar disk which is thought to be the cradle of planets. IAU Symposium 243 highlights the latest developments in understanding the structure and evolution of the star-disk interaction region in young stars, a critical component of our knowledge of star and planetary system formation processes. Discussions review the physical processes thought to be at work at the star-disk interface, confront the predictions of the latest numerical and analytical magnetohydrodynamic models of star-disk-jet systems with observations, and explore the consequences of these processes for stellar angular momentum evolution and inner disk structure. The most recent observational results, computer simulations and theoretical developments in this active field of research are included to provide a unique vision into this central aspect of the star and planet formation problem. IAU S243 reviews recent developments in understanding the structure and evolution of the star-disk interaction region in young stars. The latest observational results, computer simulations and theoretical developments are included, providing a unique review of this topic that is ideal for graduate students and researchers. This item is printed on demand. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability. N° de réf. du vendeur 9780521874656
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Gebunden. Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. IAU S243 reviews recent developments in understanding the structure and evolution of the star-disk interaction region in young stars. The latest observational results, computer simulations and theoretical developments are included, providing a unique review. N° de réf. du vendeur 594766645
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