Accretion of supersonic magnetized winds onto black holes
High Energy Astrophysical Phenomena
2023-02-20 v1
Abstract
We present the accretion of magnetized supersonic winds onto a rotating black hole in three dimensions. We select representative spin-wind orientations in order to illustrate its effects on the evolution and morphology of the shock cone. The most important finding in the magnetized case, unlike the purely hydrodynamical scenario, is the formation of rarified spots where the magnetic field pressure dominates over the gas pressure. In these rarified spots we find the formation of eddies within the shock cone.
Keywords
Cite
@article{arxiv.2301.04307,
title = {Accretion of supersonic magnetized winds onto black holes},
author = {Miguel Gracia-Linares and Francisco S. Guzmán},
journal= {arXiv preprint arXiv:2301.04307},
year = {2023}
}
Comments
9 pages, 10 figures. Accepted for publication in MNRAS