Sprache: Englisch
Verlag: Dordrecht, Kluwer Academic Publ., 1994
ISBN 10: 0792333314 ISBN 13: 9780792333319
Anbieter: Antiquariat Thomas Haker GmbH & Co. KG, Berlin, Deutschland
Verbandsmitglied: GIAQ
Hardcover. 501 S.; Ill. Good condition. Note of ownership. Sprache: Englisch Gewicht in Gramm: 1235 Reprinted from Astrophysics and Space Science; Vol. 221, Nos.1-2, 1994.
Anbieter: Ria Christie Collections, Uxbridge, Vereinigtes Königreich
EUR 93,31
Anzahl: Mehr als 20 verfügbar
In den WarenkorbZustand: New. In.
Sprache: Englisch
Verlag: Springer Netherlands|Springer, Berlin, 1995
ISBN 10: 0792333314 ISBN 13: 9780792333319
Anbieter: moluna, Greven, Deutschland
EUR 104,18
Anzahl: Mehr als 20 verfügbar
In den WarenkorbZustand: New. These proceedings of a workshop held at Isle-aux-Coudres, Quebec, Canada in August 1993, provide a comprehensive, up-to- date assessment of a fundamental subject in modern stellar astrophysics. Hot, luminous stars play a crucial role in the rapid recycling .
Anbieter: Revaluation Books, Exeter, Vereinigtes Königreich
EUR 142,90
Anzahl: 2 verfügbar
In den WarenkorbHardcover. Zustand: Brand New. reprint edition. 520 pages. 10.00x6.75x1.00 inches. In Stock.
Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - These proceedings of a workshop held at Isle-aux-Coudres, Quebec, Canada in August 1993, provide a comprehensive, up-to- date assessment of a fundamental subject in modern stellar astrophysics. Hot, luminous stars play a crucial role in the rapid recycling of matter in dense regions of the Universe. The most luminous objects generate the strongest outflows of material, which in turn have a profound impact on both the interstellar medium and the underlying stars themselves. However, recent observational and theoretical advances have shown that these outflows are highly unstable and inhomogeneous. These characteristics constitute a fundamental property of the outflows that can no longer be disregarded. Instability and Variability of Hot-Star Winds provides an in-depth assessment of this important phenomenon from both an observational and a theoretical perspective. It includes up-to- date discussions of the observational diagnostics of time- dependent stellar-wind structure, the theoretical understanding of the origin of such structures, and its consequences for the process of mass loss via stellar winds. The book presents some 40 invited papers, each followed by in-depth discussions which occupied nearly half of the workshop schedule. A round-table discussion summarizes the current state of affairs. This book is suitable for researchers and graduate students studying the radiation hydrodynamics of hot-star winds and related areas of research (e.g. astrophysical flows, turbulence).