Direct Observations of the Dynamics and Variability at High Energy Emission Regions in TeV Blazars

Details Direct Observations of the Dynamics and Variability at High Energy Emission Regions in TeV Blazars Direct Observations of the Dynamics and Variability at High Energy Emission Regions in TeV Blazars

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..402..270k&link_type=abstract

Approaching Micro-Arcsecond Resolution with VSOP-2: Astrophysics and Technologies ASP Conference Series, Vol. 402, proceedings o

Astronomy and Astrophysics

Astrophysics

Scientific paper

VSOP-2 observations of ``blazars" may be part of the VSOP-2 Key Science Program for Active Galactic Nuclei. We propose VSOP-2 observations of nearby blazars together with a multi-frequency campaign observations. For example, in two nearby TeV blazars Mrk 421 and Mrk 501, the 38 micro-arcsec resolution corresponds to about 0.03 pc in linear scale, which is comparable to the size of the high energy emission region in the standard one-zone model.
We show the advantages of VSOP-2 observation of these blazars compared with previous VLBI studies, and discuss some relevant unresolved problems.

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