X-ray studies of blazars

Details X-ray studies of blazars X-ray studies of blazars

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..558..346t&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: International Symposium. AIP Conference Proceedings, Volume 558, pp. 346-357 (2001).

Astronomy and Astrophysics

Astronomy

Active And Peculiar Galaxies And Related Systems

Scientific paper

The non-thermal spectra of blazars, observed from radio to GeV/TeV γ-rays, reveal two pronounced components, both produced by radiation from energetic particles. One peaks in the IR to soft X-ray band, radiating via the synchrotron process; the other, peaking at high γ-ray energies, is produced by the Compton process. The X-ray regime is important, as it is where the emission due to both processes overlap. In this paper, results from recent multi-frequency observations of blazars are reported with emphasis on X-ray observations. .

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