The Ionization and Thermal Equilibrium of a Gas Excited by Ultraviolet Synchrotron Radiation

• Main Author: Williams, R. E.
• Other Authors: Univ Arizona, Steward Observ
• Language: en_US
• Published: Steward Observatory, The University of Arizona (Tucson, Arizona) 1966
• Subjects: Synchrotron radiation; Gas dynamics; Models; Ionization; Ultraviolet radiation
• Online Access: http://hdl.handle.net/10150/623809; http://arizona.openrepository.com/arizona/handle/10150/623809

The ionization and thermal balances are considered for a gas that is ionized by a dilute radiation field, taking into account the diffuse ionizing radiation produced by the gas. A number of models are constructed in which the electron temperature and the ionization of the elements H, He, C, N, 0, Ne, and Mg are determined for optically thin and optically thick gases ionized by ultraviolet synchrotron radiation under different conditions. Conclusions are then drawn about the general characteristics of ionization by synchrotron radiation. It is shown that, in an optically thin gas, because of the insensitive frequency- dependence of synchrotron radiation each element occupies a number of different stages of ionization at any one point in the gas. It is also shown that in an optically thick gas the heavy elements remain ionized to much greater distances from the source than hydrogen and helium, and that the gas becomes thermally unstable when H and He have become almost completely neutral. In addition, observations of the emission -line intensities of the Crab Nebula are compared with a model of this object. Considerable disagreement exists between the observed and predicted intensities, and possible reasons for the discrepancy are discussed.