Hydrodynamic Simulations of Double-Bent Radio Sources

Details Hydrodynamic Simulations of Double-Bent Radio Sources Hydrodynamic Simulations of Double-Bent Radio Sources

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21714235m&link_type=abstract

American Astronomical Society, AAS Meeting #217, #142.35; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

Using three-dimensional hydrodynamic modeling, we simulate the development and evolution of Active Galactic Nuclei in galaxy groups in order to better understand the relationship between jet curvature and various properties of the Intergalactic Medium and of the AGN itself, with an emphasis on the use of radius of curvature as a density probe of the IGM.

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