Abstract
With the outcoming of high angular resolution imaging and 3D spectrographic facilities (HST, TIGER-OASIS [1] 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 hydrodynamical 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 hydrodynamical models including a good description of atomic physic processes (using photoionisation routines from the code MAPPINGS [2]).
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References
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© 1996 International Astronomical Union
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Ferruit, P., Binette, L., Pecontal, E. (1996). ISM/Radio Material Interaction Modeling. In: Ekers, R., Fanti, C., Padrielli, L. (eds) Extragalactic Radio Sources. International Astronomical Union, vol 175. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0295-4_167
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DOI: https://doi.org/10.1007/978-94-009-0295-4_167
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