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Monthly Notices of the Royal Astronomical Society, 2010
We use smoothed particle hydrodynamics (SPH) to simulate a head-on collision between two physically dissimilar clouds, and investigate the dynamical stability of the post-collision bow-shock. The shock-front appears susceptible to a number of hydrodynamical instabilities such as the Kelvin―Helmholtz instability, the Rayleigh-Taylor instability, and the
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We use smoothed particle hydrodynamics (SPH) to simulate a head-on collision between two physically dissimilar clouds, and investigate the dynamical stability of the post-collision bow-shock. The shock-front appears susceptible to a number of hydrodynamical instabilities such as the Kelvin―Helmholtz instability, the Rayleigh-Taylor instability, and the
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Interstellar medium magnetic field in bow shock modelling
Aircraft Engineering and Aerospace Technology, 2018Romana Ratkiewicz
exaly