MHD Simulations of Clusters of Galaxies Including Radiative Cooling View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

2007

AUTHORS

N. Asai , N. Fukuda , R. Matsumoto

ABSTRACT

We carried out 2D and 3D magnetohydrodynamic simulations including radiative cooling and anisotropic thermal conduction of a magnetically turbulent intracluster medium. In 3D simulations, we found that magnetic pressure increases by a factor of 2 at 1.4 Gyr because magnetic fields accumulate in the center along with the plasma contracting by the cooling instability. In 2D simulations including thermal conduction, we found that a low temperature region exists along the loop-shaped magnetic field lines. Thus, the restriction of thermal conduction across magnetic field lines enables the coexistence of hot and cool plasmas in cluster cores. More... »

PAGES

228-230

Book

TITLE

Heating versus Cooling in Galaxies and Clusters of Galaxies

ISBN

978-3-540-73483-3
978-3-540-73484-0

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-3-540-73484-0_40

DOI

http://dx.doi.org/10.1007/978-3-540-73484-0_40

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1008185425


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