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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Evidence That Wolf-Rayet Stars are Pre-Main Sequence Objectsloud, and that their rate of mass loss is moderate. These properties are consistent with Wolf-Rayet stars being young objects recently arrived on the main sequence rather than the evolved, peeled-down remnants of massive stars.

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A Statistical Study of Main Sequence A and F Stars: Testing the Main Sequence Mass Loss Hypothesis rotation has been suggested by Willson, Bowen, and Struck-Marcell (=WBS, 1987). These stars would evolve down the main sequence on a timescale that is less than or on the order of the nuclear evolution timescale. The mass loss process would end when the pulsation ends and/or when the rotation is braked.

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Angular Momentum and Mass Loss for Hot Stars978-94-009-2105-4Series ISSN 1389-2185

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https://doi.org/10.1007/978-3-642-28845-6“dynamical phenomena in stars and circumstellar envelopes”. Here I review the justification for the series and for the topic selected for this meeting, and note some relevant recent developments in our understanding of connections between angular momentum and mass loss for stars more massive than the Sun.

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https://doi.org/10.1007/978-3-030-01542-8 rotation has been suggested by Willson, Bowen, and Struck-Marcell (=WBS, 1987). These stars would evolve down the main sequence on a timescale that is less than or on the order of the nuclear evolution timescale. The mass loss process would end when the pulsation ends and/or when the rotation is braked.