Time of establishment of ionization equilibrium in a hot rarefied gas

Details Time of establishment of ionization equilibrium in a hot rarefied gas Time of establishment of ionization equilibrium in a hot rarefied gas

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984afz....21..353s&link_type=abstract

(Astrofizika, vol. 21, Sept.-Oct. 1984, p. 353-359) Astrophysics (ISSN 0571-7132), vol. 20, no. 5, March 1985, p. 544-548. Trans

Astronomy and Astrophysics

Astrophysics

Astrophysics, Electron Gas, High Temperature Gases, Ionized Gases, Rarefied Gases, Thermodynamic Equilibrium, Electron Energy, Galactic Clusters, Ion Concentration, Solar Flares, Supernova Remnants, Temperature Dependence

Scientific paper

The time required for establishment of ionization equilibrium in a hot rarefied gas is calculated. It is shown that strong deviations from the state of ionization equilibrium must be expected in chromospheric flares and in supernova remnants. In addition, a galaxy moving in a cluster of galaxies must leave a wake with a nonequilibrium ionization state that exists for more than 10 to the 8th - 10 to the 9th yr.

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