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thermal plasma (Raymond-Smith - He and metal abundances)

         

displaymath18141

with the tabled cooling function tex2html_wrap_inline18143 and the normalization A.

Note:The emissivity is calculated for "cosmic" abundances [Raymond and Smith1977]. If no special table is created the program uses the table exsas_cal:thbrsm. A red shift can be given.
    rsms(1,2,3,4)
 

tabular6762

   


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