Multiband VLBI observations of CTA 102.

Details Multiband VLBI observations of CTA 102. Multiband VLBI observations of CTA 102.

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...310...66r&link_type=abstract

Astronomy and Astrophysics, v.310, p.66-74

Astronomy and Astrophysics

Astrophysics

10

Galaxies: Active, Galaxies: Jets, Quasars: Cta102

Scientific paper

The source CTA102, known to exhibit low frequency variability, has been observed at six epochs (three at λ32cm, two at λ18cm, and one at λ1.3cm) with intercontinental VLBI arrays. On the basis of the changes observed in the structure, we believe that the flux density variations at these wavelengths are due to intrinsic processes and not due to interstellar scintillation. This source exhibits behaviour suggestive of being expanding with a very high apparent transverse velocity.

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