The spectral evolution of superluminal radio knots: A shock-in-jet model with prolonged energy supply

Details The spectral evolution of superluminal radio knots: A shock-in-jet model with prolonged energy supply The spectral evolution of superluminal radio knots: A shock-in-jet model with prolonged energy supply

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996cha%26a..20..281q&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 20, Issue 3, p. 281-290.

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

In this paper a jet-shock model is proposed which includes a continuous supply of energy and adiabatic expansion of the plasma behind the shock. Our model calculations reproduce the three-stage evolution of the turnover flux-frequency curve, observed in the superluminal knot C4 of 3C,345. By considering a high-energy cutoff in the input electron spectrum, the steepening of the spectrum for υ ≿ 20 GHz, observed in C4, is also reproduced.

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