Mapping Blazars' Inner Jets Through Multiwavelength Observations

Details Mapping Blazars' Inner Jets Through Multiwavelength Observations Mapping Blazars' Inner Jets Through Multiwavelength Observations

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aprs.conf..227s&link_type=abstract

Astrophysical Phenomena Revealed by Space VLBI, Proceedings of the VSOP Symposium, held at the Institute of Space and astronauti

Physics

1

Scientific paper

Being dominated by non-thermal emission from aligned relativistic jets, blazars allow us to elucidate the physics of extragalactic jets, and, ultimately, how energy is extracted from the central black hole in radio-loud AGNs. Crucial information is provided by blazars' spectral energy distributions from radio to gamma-rays, their trends with luminosity, and correlated multifrequency variability. I will review recent results from multiwavelength monitorings of blazars which provide us with a close look to jets' inner regions.

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