Non-Equilibrium X-Ray Emission from Young Supernova Remnants
<p>A computer model (NIE model) has been developed to predict the the x-ray spectra from the hot (10<sup>6-8</sup> K), shock-heated plasmas that are found in the remnants of supernovae. The model accounts for the lack of collisional ionization equilibrium and for the possible lack...
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Format: | Others |
Language: | en |
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1983
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Online Access: | https://thesis.library.caltech.edu/10453/2/Nugent%20Jr_JJ_1983.pdf Nugent, John Joseph, Jr. (1983) Non-Equilibrium X-Ray Emission from Young Supernova Remnants. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/mees-s868. https://resolver.caltech.edu/CaltechTHESIS:09252017-104936539 <https://resolver.caltech.edu/CaltechTHESIS:09252017-104936539> |
Internet
https://thesis.library.caltech.edu/10453/2/Nugent%20Jr_JJ_1983.pdfNugent, John Joseph, Jr. (1983) Non-Equilibrium X-Ray Emission from Young Supernova Remnants. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/mees-s868. https://resolver.caltech.edu/CaltechTHESIS:09252017-104936539 <https://resolver.caltech.edu/CaltechTHESIS:09252017-104936539>