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<H1><A NAME="SECTION001320000000000000000">
Astrophysical Context</A>
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<P>
The process of absorption line formation in the intersteller medium has been
described in detail by several authors (e.g. Str&#246;mgren 1948, Spitzer 1978).
Here we shall give only the basic formulae and the variables to which the 
user has access in order to make the notations used in the program precise. 

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<LI><A NAME="tex2html3668"
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<LI><A NAME="tex2html3669"
 HREF="node181.html">Optical Depth</A>
<LI><A NAME="tex2html3670"
 HREF="node182.html">Broadening Function</A>
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<LI><A NAME="tex2html3671"
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<ADDRESS>
<I>Petra Nass</I>
<BR><I>1999-06-15</I>
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