Table 1:
Consequences for the CRp scaling parameter
and
by comparing the integrated flux above 730 GeV to HEGRA data of the radio
galaxy M 87 within the innermost two data points corresponding to
.
The spatial distribution of CRp is given by the isobaric,
the adiabatic, and the diffusion model, respectively (see
Sect. 3).
In the first two cases the values are calculated for a CRp population with
and without lower cutoff
while in the latter case two
different lifetimes of the source have been considered. Note that the
averaged CRp luminosity
scales with
.
and
by comparing the integrated flux above 730 GeV to HEGRA data of the radio
galaxy M 87 within the innermost two data points corresponding to
.
The spatial distribution of CRp is given by the isobaric,
the adiabatic, and the diffusion model, respectively (see
Sect. 
while in the latter case two
different lifetimes of the source have been considered. Note that the
averaged CRp luminosity
scales with
.