脱离
发表于 2025-3-23 11:47:07
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沉着
发表于 2025-3-23 17:01:08
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特别容易碎
发表于 2025-3-23 21:57:12
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.
转向
发表于 2025-3-23 23:57:46
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.
轨道
发表于 2025-3-24 03:45:31
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Shuttle
发表于 2025-3-24 08:17:16
Angular Momentum and Mass Loss for Hot Stars978-94-009-2105-4Series ISSN 1389-2185
maverick
发表于 2025-3-24 11:55:34
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.
engrossed
发表于 2025-3-24 15:22:02
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Coronation
发表于 2025-3-24 22:22:12
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INTER
发表于 2025-3-25 02:39:54
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.