Space VLBI observations of gamma-ray sources

Details Space VLBI observations of gamma-ray sources Space VLBI observations of gamma-ray sources

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..510..367e&link_type=abstract

THE FIFTH COMPTON SYMPOSIUM. AIP Conference Proceedings, Volume 510, pp. 367-371 (2000).

Astronomy and Astrophysics

Astronomy

Gamma-Ray Sources, Gamma-Ray Bursts, Active And Peculiar Galaxies And Related Systems, Radio, Microwave

Scientific paper

The radio astronomy satellite HALCA, launched in February 1997, is the main element of the VLBI Space Observatory Program (VSOP) which enables images to be made at 1.6 GHz and 5 GHz with resolutions up to three times higher than can be obtained from ground VLBI. Most VSOP observations are of compact, radio-loud flat-spectrum extragalactic sources, with many of the identified CGRO gamma-ray sources already having been observed. In this paper VSOP observations of gamma-ray sources are reviewed. .

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