3C279 Results Derived from Two-Frequency VSOP Observations

Details 3C279 Results Derived from Two-Frequency VSOP Observations 3C279 Results Derived from Two-Frequency VSOP Observations

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aprs.conf...25h&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 series of VSOP observations of 3C279 have been made at 1.6 and 5GHz during the AO1 and AO2 periods. The milli-arcsecond scale structure of 3C279 is dominated by the core and the jet component C4. The spectral index map obtained from the 1.6GHz VSOP and 5GHz ground-only maps shows an inverted spectrum at the core indicating synchrotron self-absorption. Due to the evolution of the VSOP beam, AO2 images show much finer details of parsec-scale components.

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