Descripción
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I present simulations of stellar jets interacting the interstellar medium. I will first briefly describe HERACLES, a 3D radiation-hydrodynamics code, and the model of jets used in these simulations. I will then highlight the crucial differences between considering just cooling or radiative transfer to model such a problem. In particular, I will show that radiation-hydrodynamics could lead to the jet collimation and the creation of a secundary jet. | |
Internacional
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Si |
ISSN o ISBN
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Entidad relacionada
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Radiative Transfer Working Group of the European Interferometry Initiative |
Nacionalidad Entidad
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Sin nacionalidad |
Lugar del congreso
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Lyon (France) |