Graphics Interfaces and Remote Numerical Simulations of the Interaction of High Velocity Clouds with Galactic Disks

Details Graphics Interfaces and Remote Numerical Simulations of the Interaction of High Velocity Clouds with Galactic Disks Graphics Interfaces and Remote Numerical Simulations of the Interaction of High Velocity Clouds with Galactic Disks

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..396..273h&link_type=abstract

Formation and Evolution of Galaxy Disks ASP Conference Series, Vol. 396, Proceedings of the conference held 1-5 October, 2007 at

Astronomy and Astrophysics

Astronomy

Scientific paper

The interaction of high velocity clouds (HVC) with the interstellar medium (ISM) plays an important role in the evolution of galactic structure tep{S99,S07}. In this work, we present preliminary results of the Virtual Catalog of Remote Numerical Simulations associated with the evolution of HVC in a magnetized medium. Here we explain in detail the development of the graphic user interface to perform web-based, remote numerical simulations and database, respectively.

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