Observations of Relativistic Outflow in AGN and the Brightness Temperature of Synchrotron Sources

Details Observations of Relativistic Outflow in AGN and the Brightness Temperature of Synchrotron Sources Observations of Relativistic Outflow in AGN and the Brightness Temperature of Synchrotron Sources

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aprs.conf..159k&link_type=abstract

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

Astronomy and Astrophysics

Astrophysics

10

Scientific paper

VLBA observations over a five year period are used to discuss the
outflow of relativistic plasma from the center of quasars and AGN. The
distribution of apparent linear velocity has a tail indicating pattern
velocities up to 20c, but there is little evidence for corresponding
Doppler boosting of the flux density.

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