Equilibrium of gas in the gravitational field of cD galaxies

Details Equilibrium of gas in the gravitational field of cD galaxies Equilibrium of gas in the gravitational field of cD galaxies

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986afz....24...57v&link_type=abstract

(Astrofizika, vol. 24, Jan.-Feb. 1986, p. 57-64) Astrophysics (ISSN 0571-7132), vol. 24, no. 1, July 1986, p. 34-39. Translation

Astronomy and Astrophysics

Astrophysics

2

Cosmic Gases, Equilibrium Equations, Galactic Clusters, Gas Dynamics, Gravitational Fields, Conductive Heat Transfer, Electron Energy, Radiative Heat Transfer

Scientific paper

The possibility of applying solutions to the equations of hydrostatic and energy equilibrium to describe the distribution of gas in the gravitational field of cD galaxies is investigated. It is shown that the condition of energy equilibrium without allowance for the energy fluxes is most probably not satisfied. The radiation losses in the center of a cD galaxy can in this case be compensated by electron heat conduction and matter fluxes from the hotter exterior regions of the cD galaxies.

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