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R.L. Porter, G.J. Ferland (University of Kentucky), S.B. Kraemer (Catholic University of America)
Using the plasma simulation code Cloudy, we calculate x-ray emission from several of the more abundant ions of the Helium-like isoelectronic sequence, and present new predictions for standard diagnostics. We explore a range of conditions and compare with previous work and observations.
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Bulletin of the American Astronomical Society, 37 #4
© 2005. The American Astronomical Soceity.