Intermediate Scale Theory Use Cases

Description of two examples of intermediate scale numerical simulations of very different astrophysical problems. The first problem addresses the evolution of globular clusters, where the dynamical and stellar evolution is followed for every star in the cluster. The second problem describes the evolution of extragalactic jets, both energetic FRII MHD jets and less energetic FRI MHD jets in clusters of galaxies that form buoyant bubbles in the intracluster medium.

Topic attachments
I Attachment Action Size Date Who Comment
Quicktime moviempeg HB5ka.mpeg manage 1839.5 K 2005-10-06 - 09:27 PeterTeuben Magnetic field
Quicktime moviempeg HB5kc.mpeg manage 1498.6 K 2005-10-06 - 09:29 PeterTeuben Tracer of radio source material
PowerPointppt IVOATheory0905.ppt manage 908.0 K 2005-10-06 - 09:26 PeterTeuben IVOA oct 2005 presentation
Topic revision: r1 - 2005-10-06 - PeterTeuben
This site is powered by the TWiki collaboration platformCopyright © 2008-2019 by the contributing authors. All material on this collaboration platform is the property of the contributing authors.
Ideas, requests, problems regarding TWiki? Send feedback