32 citations · 101 across the 14 of their papers we have counts for
7 papers · 1 filter
Virtual Spectro, a tool for spectroscopic signatures of plasma
Michel Busquet
We present here the tool "Virtual Spectro", a post-processor for spectroscopics analysis of hydrodynamic codes. We describe purpose and method of this tool, and the first applicati…
Comments on "Experimental study of radiative shocks at PALS facility" by Chantal Stehle et al. (arXiv:1003.2739v1 [astro-ph.SR])
Michel Busquet
Discussion on paper "Experimental study of radiative shocks at PALS facility" by C. Stehle et al (arXiv:1003.2739v1 [astro-ph.SR]) is presented, findings are questioned.
Comparison of Fe and Ni opacity calculations for a better understanding of pulsating stellar envelopes
D. Gilles, S. Turck-Chièze, G. Loisel +19
Opacity is an important ingredient of the evolution of stars. The calculation of opacity coefficients is complicated by the fact that the plasma contains partially ionized heavy io…
Iron and Nickel spectral opacity calculations in conditions relevant for pulsating stellar envelopes and experiments
D. Gilles, S. Turck-Chièze, M. Busquet +18
Seismology of stars is strongly developing. To address this question we have formed an international collaboration OPAC to perform specific experimental measurements, compare opaci…
On the influence of opacity variation on spatial structure of radiative shocks
M. Busquet, M. Klapisch, F. Thais
We provide a theoretical analysis of Radiative Shocks, defined as supercritical shocks accompanied by an ionization wave in front of the density jump. In particular, we look at the…
Theoretical and experimental activities on opacities for a good interpretation of seismic stellar probes
S Turck-Chièze, G Loisel, D Gilles +23
Opacity calculations are basic ingredients of stellar modelling. They play a crucial role in the interpretation of acoustic modes detected by SoHO, COROT and KEPLER. In this review…
Radiative properties of stellar plasmas and open challenges
S. Turck-Chièze, G. Loisel, D. Gilles +24
The lifetime of solar-like stars, the envelope structure of more massive stars, and stellar acoustic frequencies largely depend on the radiative properties of the stellar plasma. U…