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20032008
most citedThe turbulent destruction of clouds - I. A k-epsilon treatment of turbulence in 2D models of adiabatic shock-cloud interactions

74 citations · 94 across the 2 of their papers we have counts for

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astro-ph200874 cited

The turbulent destruction of clouds - I. A k-epsilon treatment of turbulence in 2D models of adiabatic shock-cloud interactions

J. M. Pittard, S. A. E. G. Falle, T. W. Hartquist +1

The interaction of a shock with a cloud has been extensively studied in the literature, where the effects of magnetic fields, radiative cooling and thermal conduction have been con…

astro-ph200620 cited

The tails in the Helix Nebula NGC 7293

J. E. Dyson, J. M. Pittard, J. Meaburn +1

We have examined a stream-source model for the production of the cometary tails observed in the Helix Nebula NGC 7293 in which a transonic or moderately supersonic stream of ionize…

astro-ph2005

Dynamical and Pressure Structures in Winds with Multiple Embedded Evaporating Clumps I. 2D Numerical Simulations

J. M. Pittard, J. E. Dyson, S. A. E. G. Falle +1

Because of its key role in feedback in star formation and galaxy formation, we examine the nature of the interaction of a flow with discrete sources of mass injection. We show the…

astro-ph2005

The Shocking Properties of Supersonic Flows: Dependence of the Thermal Overstability on M, alpha, and T_c/T_0

J. M. Pittard, M. S. Dobson, R. H. Durisen +3

We investigate the Mach number dependence of the radiative overstability of shocks. We find that the stability of radiative shocks increases with decreasing Mach number, with the r…

astro-ph2003

The Formation of Broad Emission Line Regions in Supernova-QSO Wind Interactions II. 2D Calculations

J. M. Pittard, J. E. Dyson, S. A. E. G. Falle +1

One aspect of supernova remnant evolution that is relatively unstudied is the influence of an AGN environment. A high density ambient medium and a nearby powerful continuum source…