Cosmic ray acceleration of gas in active galactic nuclei
Dynamical models of Seyfert nuclei and quasi-stellar objects are presented. The central energy source often postulated for these active objects provides a means of heating and ionizing the nuclear gas, and also exerts an outward force on the gas. Since the gas will be fully ionized, it will be nearl...
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Language: | English |
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2010
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Online Access: | http://hdl.handle.net/2429/19617 |