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thermal plasma (Raymond-Smith - individual abundances)

       

displaymath18157

with the calculated cooling function tex2html_wrap_inline18159 and the normalization amplitude A.

rsma(1,2,3,4,5,6,7,8,9,10,11,12,13,14)
 

tabular6781

   

Note:All abundances are given relative to the "cosmic" abundances. For defaults see [Raymond and Smith1977]. A redshift can be given. This function should be used if single abundances should be fitted. It almost does the same as the model rsmf, only faster. The table exsas_cal:thbrall from the calibration has to be specified under the general key word SPECTRAL_MODEL_FILE of the corresponding spectral parameter file.
   



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