Comparison of Total Flux and VLBI Properties of a Sample of Fifteen AGN at 22 GHz

Details Comparison of Total Flux and VLBI Properties of a Sample of Fifteen AGN at 22 GHz Comparison of Total Flux and VLBI Properties of a Sample of Fifteen AGN at 22 GHz

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aprs.conf..321w&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

Scientific paper

A sample of 15 bright AGN has been observed at 22GHz with three epoch global VLBI observations. The sample consists of all the sources in the complete 2 Jy catalogue of Valtaoja et al. (1992) that were still unobserved at 22GHz VLBI in 1992 when the project started. We have started to compare source parameters (Doppler boost factors, shock sizes, and brightness temperatures) derived from total flux density (TFD) monitoring data and/or from VLBI.

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