A thermal bremsstrahlung spectrum based on the Kellogg, Baldwin & Koch
(ApJ 199, 299) polynomial fits to the Karzas & Latter numerical
values. A routine from Kurucz is used in cases of high temperature. The
He abundance is assumed to be 8.5
Keith Arnaud (kaa@genji.gsfc.nasa.gov)
Mon Sep 18 14:36:38 EDT 1995
