Radiative MHD simulations of the jets from RW Aurigae

Details Radiative MHD simulations of the jets from RW Aurigae Radiative MHD simulations of the jets from RW Aurigae

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..275..410t&link_type=abstract

Jets at all Scales, Proceedings of the International Astronomical Union, IAU Symposium, Volume 275, p. 410-411

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Computation

Atomic Processes, Mhd, Plasmas, Radiation Mechanisms: Thermal, Shock Waves, Stars: Winds, Outflows

Scientific paper

The MHD simulations of stellar jets recently included complex models of radiative emission computation, allowing for better predictions in terms of emission line ratios. Employing also Adaptive Mesh Refinement, the large-scale propagation of jets could be followed. The simulation of multiple shockwaves originating in perturbations close to the jet origin and travelling along the jet beam allows for the construction of synthetic emission maps at various wavelengths, to be directly compared to observations. We apply this procedure for the jets originating from RW Aurigae.

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