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Mathematisch-Naturwissenschaftliche Fakultät
Fachgruppe Physik

I. Physikalisches Institut

Synthetic spectra from chemical calculations

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The chemical code Saptarsy has been developed to calculate chemical evolution in star-forming regions.  It has the ability to calculate synthetic spectra that can be compared to observations, but this is a very time consuming process.  The thesis is about developing a faster, if less acurate, method based on XCLASS, and to apply this to a parameter study for typical star formation conditions.