تقرير
Magnetized Rotating Isothermal Winds
العنوان: | Magnetized Rotating Isothermal Winds |
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المؤلفون: | Raives, Matthias J., Coleman, Matthew S. B., Thompson, Todd A. |
المصدر: | MNRAS, 526, 3, 4418-4434 (2023) |
سنة النشر: | 2023 |
المجموعة: | Astrophysics |
مصطلحات موضوعية: | Astrophysics - Solar and Stellar Astrophysics, Astrophysics - High Energy Astrophysical Phenomena |
الوصف: | We consider the general problem of a Parker-type non-relativistic isothermal wind from a rotating and magnetic star. Using the magnetohydrodynamics (MHD) code athena++, we construct an array of simulations in the stellar rotation rate $\Omega_\ast$ and the isothermal sound speed $c_T$, and calculate the mass, angular momentum, and energy loss rates across this parameter space. We also briefly consider the three dimensional case, with misaligned magnetic and rotation axes. We discuss applications of our results to the spindown of normal stars, highly-irradiated exoplanets, and to nascent highly-magnetic and rapidly-rotating neutron stars born in massive star core collapse.8 Comment: 19 pages, 13 figures; v2: published version after minor revisions |
نوع الوثيقة: | Working Paper |
DOI: | 10.1093/mnras/stad301688 |
الوصول الحر: | http://arxiv.org/abs/2302.05462Test |
رقم الانضمام: | edsarx.2302.05462 |
قاعدة البيانات: | arXiv |
DOI: | 10.1093/mnras/stad301688 |
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