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Historical perspective on astrophysical MHD simulations

Published online by Cambridge University Press:  27 April 2011

Michael L. Norman
Michael L. Norman*
Affiliation:
Center for Astrophysics and Space Sciences San Diego Supercomputer Center, La Jolla, CA 92093, USA email: [email protected]
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Abstract

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This contribution contains the introductory remarks that I presented at IAU Symposium 270 on “Computational Star Formation” held in Barcelona, Spain, May 31–June 4, 2010. I discuss the historical development of numerical MHD methods in astrophysics from a personal perspective. The recent advent of robust, higher-order accurate MHD algorithms and adaptive mesh refinement numerical simulations promises to greatly improve our understanding of the role of magnetic fields in star formation.

Keywords

ISM: star formationISM: magnetic fieldsmethods: numerical
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S270: Computational Star Formation , May 2010 , pp. 7 - 17
Copyright
Copyright © International Astronomical Union 2011

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