Simulations of Double-Bent Radio Sources

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

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21533601m&link_type=abstract

American Astronomical Society, AAS Meeting #215, #336.01; Bulletin of the American Astronomical Society, Vol. 42, p.439

Astronomy and Astrophysics

Astronomy

Scientific paper

We are performing hydrodynamic simulations of non-central AGN sources moving through galaxy clusters. The simulations are intended to reproduce the findings of X-ray and radio observations and to determine the effect of jet power and motion on radius of curvature for double-bent radio tails, heating of the outer cluster, and the evolution of radio bubbles over time.

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