Simulations of the flux contours of astrophysical jets

Details Simulations of the flux contours of astrophysical jets Simulations of the flux contours of astrophysical jets

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...223..369z&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 223, no. 1-2, Oct. 1989, p. 369-374.

Astronomy and Astrophysics

Astronomy

2

Extragalactic Radio Sources, Herbig-Haro Objects, Radio Jets (Astronomy), Astronomical Spectroscopy, Elliptical Galaxies, Emissivity, Kelvin-Helmholtz Instability, Relativistic Particles, Synchrotron Radiation

Scientific paper

The observed morphological features of extragalactic jets and Herbig-Haro objects include wiggles and pinches. The theory of the Kelvin-Helmholtz instabilities is applied to trace the jet's pattern. To obtain realistic plots, a certain level of noise is introduced. Superposed on the blob's trajectory, computer simulations are produced for the emitted flux and the frequency of emission of the electrons that diffuse away from the active zones. Simulations of the flux from the Herbig-Haro objects are obtained, introducing variuos laws for the blob's containment.

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