Magnetized rotating isothermal winds-Reference-Cited by-同舟云学术

Magnetized rotating isothermal winds

Published:2023-10-05 Issue:3 Volume:526 Page:4418-4434
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Raives Matthias J¹²³^ORCID,Coleman Matthew S B⁴⁵,Thompson Todd A²³⁶^ORCID

Affiliation:

1. The Observatories of the Carnegie Institution for Science , 813 Santa Barbara St, Pasadena, CA 91101 , USA

2. Department of Astronomy, The Ohio State University , Columbus, OH 43210 , USA

3. Center for Cosmology and Astroparticle Physics, The Ohio State University , Columbus, OH 43210 , USA

4. Department of Astrophysical Sciences , 4 Ivy Lane, Princeton University, Princeton, NJ 08540 , USA

5. Department of Physics and Engineering Physics, Stevens Institute of Technology, Castle Point on the Hudson , Hoboken, NJ 07030 , USA

6. Department of Physics, The Ohio State University , Columbus, OH 43210 , USA

Abstract

ABSTRACT We consider the general problem of a Parker-type non-relativistic isothermal wind from a rotating and magnetic star. Using the magnetohydrodynamics code athena++, we construct an array of simulations in the stellar rotation rate Ω* and the isothermal sound speed cT, and calculate the mass, angular momentum, and energy loss rates across this parameter space. We also briefly consider the 3D case, with misaligned magnetic and rotation axes. We discuss applications of our results to the spin-down of normal stars, highly irradiated exoplanets, and to nascent highly magnetic and rapidly rotating neutron stars born in massive star core-collapse.

Funder

NASA

U.S. Department of Energy

National Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stad3016/51894522/stad3016.pdf

Reference67 articles.

1. The Magnetorotational Instability in Core‐Collapse Supernova Explosions