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Theory, observation and experiment: stellar hydrodynamics

Published online by Cambridge University Press:  25 May 2016

David Arnett
David Arnett*
Affiliation:
Steward Observatory, University of Arizona, Tucson AZ 85721, USA

Abstract

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Computer technology now allows two dimensional (2D) simulations, with complex microphysics, of stellar hydrodynamics and evolutionary sequences, and holds the promise for 3D. Careful validation of astrophysical methods, by laboratory experiment, by critical comparison of numerical and analytical methods, and by observation are necessary for the development of simulation methods with reliable predictive capability. Recent and surprising results from isotopic patterns in pre-solar grains, 2D hydrodynamic simulations of stellar evolution, and laser tests and computer simulations of Richtmeyer-Meshkov and Rayleigh-Taylor instabilities will be discussed, and related to stellar evolution and supernovae.

Type
Evolved Stars
Information
Symposium - International Astronomical Union , Volume 189: Fundamental Stellar Properties: The Interaction Between Observation and Theory , 1997 , pp. 389 - 394
Copyright
Copyright © Kluwer 1997 

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