Titlebook: Angular Momentum and Mass Loss for Hot Stars; L. A. Willson,R. Stalio Book 1990 Kluwer Academic Publishers 1990 Population.Variation.astro

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Earth System Science in the Anthropocene relatively high mass loss and rotation rates of these stars provide a strong indication that angular momentum loss might play a major role in their evolution, and might even be the source for their paradoxical active phenomena.

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https://doi.org/10.1007/978-3-642-28845-6their huge mass ejections is also discussed. Finally, a few possible evidences for rotationally or tidally induced mixing in massive O-stars are presented, suggesting that some very massive stars may evolve close to homogeneity.

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Advances in Science, Technology & Innovationsuch a wind model is constructed, and how it leads to a wind which is slow and dense in the equatorial regions and fast and tenuous along the poles. I will also describe the limitations of the model and observational evidence which cannot yet be explained by models of this type.

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Advances in Science, Technology & Innovation variations have a noticeable effect on observed line profiles only if the pole is not too far from the center of the visible stellar disk. Therefore, the phenomenon provides an easy-to-use criterion for the identification of (rapidly rotating) stars seen at small to intermediate inclination angles.

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