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Astron. Astrophys. 358, 104-112 (2000) Appendix A: debeaming and the broad band spectral slopes
In the case of a one-component model, and under the assumption that
the local spectral indices are constant, we can derive the
transformation law for the change of the spectral slope due to
relativistic beaming. If the flux density in the frame comoving with
the emitting region is where which can be written as where ![]() ![]() ![]() ![]() © European Southern Observatory (ESO) 2000 Online publication: June 26, 2000 ![]() |