Gas clouds in clusters of galaxies

Details Gas clouds in clusters of galaxies Gas clouds in clusters of galaxies

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.215..453r&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 215, Aug. 1, 1985, p. 453-461.

Astronomy and Astrophysics

Astronomy

6

Galactic Clusters, Interstellar Gas, Evaporation, Gravitational Collapse, H Beta Line, Radiative Heat Transfer, X Rays

Scientific paper

Various dynamical considerations are applied to show that clouds of gas at temperatures in the range of 10 to the fourth-10 to the 7th K probably cannot coexist with hotter diffuse gas in galaxy clusters, unless heat conduction is drastically reduced by magnetic fields. The relative contribution of such clouds to the virial cluster mass is shown to be of the order of 0.01 or less.

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