Mass Loss from Stars.pdf

Mass Loss from Stars

Proceedings from the Second Trieste Colloquium on Astrophysics, September 12-17, 1968

MASS LOSS FROM STARS' B~ RAY WEYMANN Steward Observatory, University of Arizona, Tucson, Arizona CONTENTS INTRODUCTION 97 EVIDENCE FOR ... Mass loss processes are a key uncertainty in the evolution of massive stars. They determine the amount of mass and angular momentum retained by the star, ...

5.94 MB DATEIGRÖSSE
9401034079 ISBN
Englisch SPRACHE
Mass Loss from Stars.pdf

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We plan to study the influence of individual approximations that can preclude correct mass-loss rate predictions. On the basis of comparison with observed wind parameters we will obtain wind models that are able to reliably predict wind mass-loss rates. These models will be used to obtain mass-loss rate formula for hot stars that can be used The Mathematics of Stellar Mass Loss on …

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Mass loss processes are a key uncertainty in the evolution of massive stars. They determine the amount of mass and angular momentum retained by the star, ...

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Mass loss of stars on the asymptotic giant … 09.01.2018 · As low- and intermediate-mass stars reach the asymptotic giant branch (AGB), they have developed into intriguing and complex objects that are major players in the cosmic gas/dust cycle. At this stage, their appearance and evolution are strongly affected by a range of dynamical processes. Large-scale convective flows bring newly-formed chemical elements to the stellar surface and, together with