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R. L. Porter, G. J. Ferland (University of Kentucky, Physics & Astronomy Dept.)
We present results from the third in a series of papers concerning the implementation of a complete model of helium-like line and continuum emission into the plasma simulation code CLOUDY. The first two papers are a general review of the methods used (including comparisons with previous works) and a discussion of all continuum processes included. The third paper is a study of the application of the code. This presentation, then, focuses on a few nebular simulations and discusses our success in reproducing observations.
The author(s) of this abstract have provided an email address for comments about the abstract: rporter@pa.uky.edu
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Bulletin of the American Astronomical Society, 35 #3
© 2003. The American Astronomical Soceity.