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ISM / Radio Material Interaction Modeling

Published online by Cambridge University Press:  25 May 2016

P. Ferruit ,
L. Binette  and
E. Pecontal
P. Ferruit
Affiliation:
CRAL Observatoire de Lyon – UMR142 9, av. Charles André − 69561 Saint-Genis-Laval Cedex, France
L. Binette
Affiliation:
CRAL Observatoire de Lyon – UMR142 9, av. Charles André − 69561 Saint-Genis-Laval Cedex, France
E. Pecontal
Affiliation:
CRAL Observatoire de Lyon – UMR142 9, av. Charles André − 69561 Saint-Genis-Laval Cedex, France

Extract

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With the outcoming of high angular resolution imaging and 3D spectrographic facilities (HST, TIGER-OASIS at the CFH Telescope…), the need of spatially resolved theoretical models of the kinematic interaction of radio material with the ISM (or the IGM for radio-galaxies) is increasing dramatically. In order to fill the gap between pure hydro dynamical models (3D approach, but very poor atomic physic) and photoionisation/shocks ones (planar description, full account for atomic physic processes), we have started to develop 2D or 3D hydro dynamical models including a good description of atomic physic processes (using photoionisation routines from the code MAPPINGS).

Type
Radio Source Modelling and Emission Mechanisms
Information
Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 465 - 466
Copyright
Copyright © Kluwer 1996 

References

1. Bacon, R., et al., 1995. A & A Supp. , 113, 347.Google Scholar
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