Heavey Iron, in Star Cluster |
| Posted by Clarence Middleton LLC (admin) on Feb 08 2006 |
The Program was designed to simulate emission line regions ranging from the intergalactic medium to the Broad Line Regions of Quasars. It can be used to predict either the structure or the observed spectrum from such regions.
My Task was to extract a certian functionality from the Cloudy software system. Document All Change, and Document all other areas of the code as well.
Last changed: Apr 26 2006 at 5:57 AM
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