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Books > Science & Mathematics > Astronomy, space & time > Galaxies, clusters, intergalactic matter

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Angular Momentum and Mass Loss for Hot Stars (Hardcover, 1990 ed.) Loot Price: R5,347
Discovery Miles 53 470
Angular Momentum and Mass Loss for Hot Stars (Hardcover, 1990 ed.): L.A. Willson, R. Stalio

Angular Momentum and Mass Loss for Hot Stars (Hardcover, 1990 ed.)

L.A. Willson, R. Stalio

Series: NATO Science Series C, 316

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Loot Price R5,347 Discovery Miles 53 470 | Repayment Terms: R501 pm x 12*

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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.

General

Imprint: Springer
Country of origin: Netherlands
Series: NATO Science Series C, 316
Release date: August 1990
First published: 1990
Editors: L.A. Willson • R. Stalio
Dimensions: 234 x 156 x 26mm (L x W x T)
Format: Hardcover
Pages: 365
Edition: 1990 ed.
ISBN-13: 978-0-7923-0881-2
Categories: Books > Science & Mathematics > Astronomy, space & time > Galaxies, clusters, intergalactic matter > General
Books > Science & Mathematics > Physics > Applied physics & special topics > Astrophysics
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LSN: 0-7923-0881-6
Barcode: 9780792308812

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