EDP Sciences Journals List
Home arrow Document
   
Issue EAS Publications Series
Volume 13, 2004
Evolution of Massive Stars, Mass Loss and Winds
Page(s) 377 - 394
DOI 10.1051/eas:2004062

Evolution of Massive Stars, Mass Loss and Winds
M. Heydari-Malayeri, Ph. Stee and J.-P. Zahn (eds)
EAS Publications Series, 13 (2004) 377-394

DOI: 10.1051/eas:2004062

Astrophysics driven by high-power lasers and radiative shocks

C. Michaut

LUTH, UMR 8102 du CNRS, Observatoire de Paris, 5 place Jules Janssen, 92195 Meudon Cedex, France.

Claire.Michaut@obspm.fr

Abstract
Astronomy and astrophysics can today produce a lot of discoveries and syntheses, driven by the convergence of sophisticated technology (advanced detectors and instrumentation, and supercomputers) with new observation platforms (VLT, Keck) and a revitalised satellite program. These advances will decisively affect many of the fundamental studies of origins, dynamics, and emission for all scales of astrophysical phenomena. Traditionally astrophysical research has been divided into observations and theoretical modelling or a combination of both. But scientists have discovered that existing models did not explain their observations of the great supernova of 1987. Since is born a closed collaboration between astrophysicists and plasma scientists leading to perform laboratory experiments motivated by the astrophysics. Start many collaborations is essential in order to progress in this new field and together astro/plasma physicists and laser bench scientists are pushing the frontiers of recreating the Universe's most exotic phenomena. The goal is to create in the laboratory a sample plasma similar to what would be found in the astronomical body, then to study its properties (radiation or thermodynamical state).



© EAS, EDP Sciences 2004


What is OpenURL?