A single internal working surface in a periodic jet

Details A single internal working surface in a periodic jet A single internal working surface in a periodic jet

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.278..990b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 278, Issue 4, pp. 990-996.

Astronomy and Astrophysics

Astronomy

12

Methods: Numerical, Ism: Jets And Outflows

Scientific paper

We present the numerical simulation of a single internal working surface which forms along the body of a supersonic jet with periodic variations in the magnitude of its velocity. The structure, the evolution and the observational properties of this flow are analysed. We make a qualitative comparison with previous analytic predictions, simulations of the complete jet and observations of Herbig-Haro jets. The apparent lag of the knots of emission with respect to the jet flow (which has been observed in some jets) can be explained by this model.

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