ASCA observations of blazars and multiband analysis

Details ASCA observations of blazars and multiband analysis ASCA observations of blazars and multiband analysis

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410.1467t&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 1467-1471 (1997).

Astronomy and Astrophysics

Astronomy

Active And Peculiar Galaxies And Related Systems, Magnitudes And Colors, Luminosities, Astronomical Observations

Scientific paper

We present results of multiband analysis for 18 blazars observed with the X-ray satellite ASCA, half of which were also observed contemporaneously with EGRET instrument onboard Compton Gamma-ray Observatory (CGRO). Our multi-band analysis suggests that the magnetic field is 0.1~1 gauss. With these values of B, we estimate γb is 103~104 for quasar-hosted blazars (QHBs), and 105 for X-ray selected BL Lac objects (HBLs).

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