Next: Source Models (normalized to
Up: Source Models (normalized to
Previous: black body (Planck spectrum)
gsef(1,2,3)
Note:For numerical reasons one must not choose the line width
too small ( keV).
This can always be done in view of the poor resolution
of X-ray detectors like the ROSAT XRT PSPC.
If you have problems/suggestions please send mail to
rosat_svc@mpe-garching.mpg.de