3D numerical simulations of a radiative Herbig-Haro jet in a supersonic side wind

Astronomy and Astrophysics – Astronomy

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Hydrodynamics, Ism: Jets And Outflows

Scientific paper

We have performed 3D numerical simulations of an over-pressurized Herbig-Haro-type jet which propagates into a sidestreaming environment. The interaction between the jet and the sidewind results in a perpendicular acceleration of the jet material, and a consequent curvature of the jet as it moves into the anisotropic medium. We find that an approximately steady configuration is achieved both for a sidewind that is perpendicular to the jet and for a sidewind inclined at 45° towards the jet source. The curvature obtained in both these models is consistent with analytic models of the jet/sidewind problem. We have also calculated Hα maps, which show an emitting sheath around the upwind (with respect to the sidewind) side of the jet beam. This emitting sheath may explain part of the observed emission from curved stellar jets.

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