|
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. MichautLUTH, 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? |

Document
BibSonomy
CiteUlike
Connotea
Del.icio.us
Digg
Facebook