On the shock wave theory of 'superluminal' radio jets

Details On the shock wave theory of 'superluminal' radio jets On the shock wave theory of 'superluminal' radio jets

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26at...20..287k&link_type=abstract

Astronomical and Astrophysical Transactions, vol. 20, Issue 2, pp.287-290

Astronomy and Astrophysics

Astronomy

Quasars, Flares, Superluminal Jets, Relativistic Shocks

Scientific paper

Superluminal parsec scale components of jets in an AGN are considered as
being parts of a shock front excited by a flare (explosion) in the
vicinity of the nucleus and moving at small angles to the direction of
sight. The influence of laminar flows (accretion and wind) is discussed,
as well as pumping from the flare region.

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