Articles liés à Angular Momentum and Mass Loss for Hot Stars
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- ÉditeurSpringer
- Date d'édition2013
- ISBN 10 9401074461
- ISBN 13 9789401074469
- ReliureLivre broché
- Nombre de pages384
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Angular Momentum and Mass Loss for Hot Stars
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Description du livre Taschenbuch. Etat : Neu. Druck auf Anfrage Neuware - Printed after ordering - Fundamental unsolved problems of stellar astrophysics include the effects of angular momentum on stellar structure and evolution, the nature and efficiency of the processes by which angular momentum is redistributed within and lost from stars, and the role that stellar rotation plays in enhancing or driving stellar mass loss. There appears to be a qualitative change in the nature and efficiency of these mechanisms near spectral type FO: hotter (more massive) stars typically retain more angular momentum at least until they reach the main sequence, while cooler stars typically spin down quickly. For the hotter stars, recent work suggests a strong link between the type of pulsation behavior, the mass loss rates, and the rotation velocity. If the same mechanisms are able to drive mass loss from the main sequence A stars, as has recently been proposed, then the current interpretations of a number of observations will be drastically affected: e. g. the ages of clusters may be incorrect by up to a factor of two, and the surface abundances of isotopes of He, Li and Be may no longer give constraints on cosmological nucleosynthesis. There are also effects on the evolution of the abundances of elements in the interstellar medium and on the general evolution of populations of stars. Thus the questions of the mechanisms of angular momentum and mass loss of stars more massive than the sun is important not only for stellar studies but for the foundations of much of modern astrophysics. N° de réf. du vendeur 9789401074469
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Angular Momentum and Mass Loss for Hot Stars (Nato Science Series C:) [Paperback ]
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Description du livre Soft Cover. Etat : new. This item is printed on demand. N° de réf. du vendeur 9789401074469
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Angular Momentum and Mass Loss for Hot Stars (Nato Science Series C:, 316)
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Description du livre Etat : New. N° de réf. du vendeur ABLIING23Apr0412070057096
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Angular Momentum and Mass Loss for Hot Stars
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Description du livre Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Proceedings of the NATO Advanced Research Workshop, Ames, Iowa, U.S.A., October 23-27, 1989 Fundamental unsolved problems of stellar astrophysics include the effects of angular momentum on stellar structure and evolution, the nature and efficiency of t. N° de réf. du vendeur 5834045
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Angular Momentum and Mass Loss for Hot Stars
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Angular Momentum and Mass Loss for Hot Stars
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Description du livre Etat : New. pp. 384 Index. N° de réf. du vendeur 26142318390
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Angular Momentum and Mass Loss for Hot Stars
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Description du livre Paperback. Etat : Brand New. 384 pages. 9.25x6.10x0.87 inches. In Stock. N° de réf. du vendeur x-9401074461
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Angular Momentum and Mass Loss for Hot Stars
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Description du livre Etat : New. Print on Demand pp. 384 49:B&W 6.14 x 9.21 in or 234 x 156 mm (Royal 8vo) Perfect Bound on White w/Gloss Lam. N° de réf. du vendeur 135013609
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Angular Momentum and Mass Loss for Hot Stars
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Description du livre Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Fundamental unsolved problems of stellar astrophysics include the effects of angular momentum on stellar structure and evolution, the nature and efficiency of the processes by which angular momentum is redistributed within and lost from stars, and the role that stellar rotation plays in enhancing or driving stellar mass loss. There appears to be a qualitative change in the nature and efficiency of these mechanisms near spectral type FO: hotter (more massive) stars typically retain more angular momentum at least until they reach the main sequence, while cooler stars typically spin down quickly. For the hotter stars, recent work suggests a strong link between the type of pulsation behavior, the mass loss rates, and the rotation velocity. If the same mechanisms are able to drive mass loss from the main sequence A stars, as has recently been proposed, then the current interpretations of a number of observations will be drastically affected: e. g. the ages of clusters may be incorrect by up to a factor of two, and the surface abundances of isotopes of He, Li and Be may no longer give constraints on cosmological nucleosynthesis. There are also effects on the evolution of the abundances of elements in the interstellar medium and on the general evolution of populations of stars. Thus the questions of the mechanisms of angular momentum and mass loss of stars more massive than the sun is important not only for stellar studies but for the foundations of much of modern astrophysics. 384 pp. Englisch. N° de réf. du vendeur 9789401074469
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