Magnetohydrodynamic interpretations of high-energy phenomena in galaxies and clusters
Kazuo Makishima; Kazuo Makishima; Department of Physics & Research Center for the Early Universe, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113, Japan
Журнал:
Plasma Physics and Controlled Fusion
Дата:
1997-05-01
Аннотация:
Energetic plasmas are found in all astrophysical environments. However, beyond the solar system, our understanding of cosmic plasma dynamics has remained quite poor. This paper presents an attempt to explore a new description of various high-energy astrophysical phenomena, observed from galaxies and galaxy clusters, in terms of plasma magnetohydrodynamics. In this context, three specific topics are described; diffuse hot plasmas filling the Milky Way, plasma acceleration by giant black holes, and hot plasmas of galaxy clusters with relevance to cosmology.
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