Physical parameters of TeV blazars

Details Physical parameters of TeV blazars Physical parameters of TeV blazars

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..558..676t&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: International Symposium. AIP Conference Proceedings, Volume 558, pp. 676-679 (2001).

Astronomy and Astrophysics

Astronomy

Active And Peculiar Galaxies And Related Systems, Radiation Mechanisms, Polarization

Scientific paper

Using multi-frequency spectra from TeV blazars at quiescent states, we obtain the physical parameters of the emission region of blazars, based on the synchrotron self-Compton model. We numerically calculate the steady-state electron energy spectrum by self-consistently taking into account radiative cooling effects with a proper account of the Klein-Nishina effects. We find that for Mrk 421, Mrk 501, and PKS 2155-304, the energy density of magnetic fields is about one order of magnitude less than that of relativistic electrons, which confirms the previous claim made analytically. .

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