Some intrinsic properties of parsec-scale radio jets

Details Some intrinsic properties of parsec-scale radio jets Some intrinsic properties of parsec-scale radio jets

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996pasa...13..103t&link_type=abstract

Publications Astronomical Society of Australia, vol. 13, no. 1, p. 103-105

Astronomy and Astrophysics

Astronomy

Jets, Radio Continuum

Scientific paper

A simple model for estimating the intrinsic flow direction and speed in the parsec-scale jets associated with extragalactic radio sources is presented. In this model radio source asymmetries are attributed to the apparent amplification caused when a relativistic jet of radiating material is somewhat aligned with the observers line-of-sight. The knots of emission commonly seen in parsec-scale radio jets are interpreted as shocks in the relativistic fluid.

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