Timeline for Strength of core-envelope coupling in stars
Current License: CC BY-SA 4.0
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Dec 30, 2018 at 21:00 | history | tweeted | twitter.com/StackAstronomy/status/1079482341880459264 | ||
Dec 30, 2018 at 6:36 | comment | added | Ken G | The problem is likely that few know the answer, indeed it might not be known by anyone. It's certainly an ongoing area of research, but it is hard to make progress purely theoretically without knowing all the variables, like magnetic field and evolutionary stage and so on. We don't even have models for star formation that could tell you the initial rotation state. So I think the question requires observations, such as asteroseismology and rotation of stellar remnants, a huge dataset with probably lots of different stories to tell. You might need to narrow down the question quite a bit! | |
Dec 30, 2018 at 6:21 | history | edited | Daddy Kropotkin | CC BY-SA 4.0 |
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Dec 29, 2018 at 13:55 | history | asked | Daddy Kropotkin | CC BY-SA 4.0 |