207 citations · 3.3k across the 108 of their papers we have counts for
27 papers · 1 filter
Momentum and energy injection by a wind-blown bubble into an inhomogeneous interstellar medium
J. M. Pittard
We investigate the effect of mass-loading from embedded clouds on the evolution of wind-blown bubbles. We use 1D hydrodynamical calculations and assume that the clouds are numerous…
Shocking interactions of supernova remnants with atomic and molecular clouds -- the interplay between shocks, thermal instability and gravity in the large cloud regime
M. M. Kupilas, J. M. Pittard, C. J. Wareing +1
Using the adaptive mesh refinement code MG, we perform 3D hydrodynamic simulations of a supernova-cloud interaction in the "large cloud regime". The cloud is initially atomic and e…
How D-type HII region expansion depends on numerical resolution
J. M. Pittard, M. M. Kupilas, C. J. Wareing
We investigate the resolution dependence of HII regions expanding past their Strömgren spheres. We find that their structure and size, and the radial momentum that they attain at a…
How to inflate a wind-blown bubble
J. M. Pittard, C. J. Wareing, M. M. Kupilas
Stellar winds are one of several ways that massive stars can affect the star formation process on local and galactic scales. In this paper we investigate the numerical resolution n…
Interactions of a shock with a molecular cloud at various stages of its evolution due to thermal instability and gravity
M. M. Kupilas, C. J. Wareing, J. M. Pittard +1
Using the adaptive mesh refinement code MG, we perform hydrodynamic simulations of the interaction of a shock with a molecular cloud evolving due to thermal instability and gravity…
Striations, integrals, hourglasses and collapse -- thermal instability driven magnetic simulations of molecular clouds
C. J. Wareing, J. M. Pittard, S. A. E. G. Falle
The MHD version of the adaptive mesh refinement (AMR) code, MG, has been employed to study the interaction of thermal instability, magnetic fields and gravity through 3D simulation…