Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989azh....66..572i&link_type=abstract
Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 66, May-June 1989, p. 572-582. In Russian.
Astronomy and Astrophysics
Astronomy
1
Gamma Ray Astronomy, High Temperature Plasmas, Iron, Metallic Plasmas, Photoionization, Bremsstrahlung, Concentration (Composition), Neutron Stars, Optical Thickness, Recombination Reactions, White Dwarf Stars
Scientific paper
A highly ionized hot plasma of an Fe-56-type heavy element in the field of hard ionizing gamma radiation is studied. Processes of ionization and recombination are discussed for a plasma consisting of fully ionized Fe XXVII and hydrogen-like Fe XXVI ions in the case of a large optical depth of the plasma with respect to photoionization by gamma-ray quanta. An equation of ionization balance is presented for a plasma in the Fe XXVII region formed around a powerful source of hard gamma-ray radiation.
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