The Bowen Fluorescence Mechanism in Planetary Nebulae and Seyfert Galaxy Nuclei
The efficiency of the Bowen fluorescence mechanism in models of planetary nebulae and Seyfert galaxy nuclei has been calculated by solving the equation of transfer for He II Ly -o( and the Bowen lines using the Feautrier method. The calculated efficiencies, which do not show significant differen...
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| Language: | en_US |
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Steward Observatory, The University of Arizona (Tucson, Arizona)
1969
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| Online Access: | http://hdl.handle.net/10150/623859 http://arizona.openrepository.com/arizona/handle/10150/623859 |