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Dust dynamics and processing in shocks

Published online by Cambridge University Press:  26 February 2009

F. Boulanger ,
C. Joblin ,
A. Jones ,
S. Madden ,
V. Guillet ,
A. Jones  and
G. Pineau des Forêts
V. Guillet
Affiliation:
Institut d'Astrophysique Spatiale, Université Paris XI, Bâtiment 121, CNRS, 91405 Orsay Cedex, France
A. Jones
Affiliation:
Institut d'Astrophysique Spatiale, Université Paris XI, Bâtiment 121, CNRS, 91405 Orsay Cedex, France
G. Pineau des Forêts
Affiliation:
Institut d'Astrophysique Spatiale, Université Paris XI, Bâtiment 121, CNRS, 91405 Orsay Cedex, France
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Abstract

The processing of dust in shocks in the interstellar medium can lead to changes in the dust to gas mass ratio and also to a radical evolution of the dust size distribution. Here we focus on the important results of numerical models that simulate the impact of shocks on the interstellar dust size distribution in molecular clouds and in the warm intercloud medium. We emphasize the necessity of detailed modelling of the grain charging processes and the grain inertia in order to unravel the complexities and consequences of the dust dynamics in shock waves.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 35: Interstellar Dust from Astronomical Observations to Fundamental Studies , 2009 , pp. 219 - 241
Copyright
© EAS, EDP Sciences, 2009

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