Some Problems with the Evolution of Gas in Clusters of Galaxies

Details Some Problems with the Evolution of Gas in Clusters of Galaxies Some Problems with the Evolution of Gas in Clusters of Galaxies

Sep 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a...101..362n&link_type=abstract

Astronomy and Astrophysics, Vol.101, P. 362, 1981

Astronomy and Astrophysics

Astrophysics

10

Scientific paper

Mixing of dynamically swept galaxy and cluster gas, so as to render one-fluid calculations completely reliable, is sufficient only if the flow Mach number is much smaller than one. The gas sweeping rate from a galaxy is connected with a number of cluster and dynamical parameters, and the one dimensional (1D) gas dynamic equations governing cluster gas evolution are rederived. Some associated problems are discussed.
The outcome of numerical experiments is presented and discussed for illustration.

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