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Numerical modeling of accretion column in polars

Published online by Cambridge University Press:  13 February 2013

C. Busschaert ,
C. Michaut ,
E. Falize  and
H.C. Nguyen
C. Busschaert
Affiliation:
LUTH, Observatoire de Paris, CNRS, Université Paris-Diderot, 92190 Meudon, France CEA-DAM-DIF, 91297 Arpajon, France
C. Michaut
Affiliation:
LUTH, Observatoire de Paris, CNRS, Université Paris-Diderot, 92190 Meudon, France
E. Falize
Affiliation:
LUTH, Observatoire de Paris, CNRS, Université Paris-Diderot, 92190 Meudon, France CEA-DAM-DIF, 91297 Arpajon, France
H.C. Nguyen
Affiliation:
LUTH, Observatoire de Paris, CNRS, Université Paris-Diderot, 92190 Meudon, France Hanoi National University of Education, 136 Xuan Thuy, Cau Giay, Ha Noi, Vietnam

Abstract

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Using powerful lasers, we are now able to produce in laboratory relevant regimes of density, temperature and velocity to create a diagnosable exact scaled model of magnetic cataclysmic variables accretion column. We present here preliminary results of a numerical modeling of these astrophysical objects which will allow us to precise the experimental setup of future experiments.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 58: ECLA - European Conference on Laboratory Astrophysics , 2012 , pp. 37 - 40
Copyright
© The Author(s) 2013

References

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