168 citations · 295 across the 6 of their papers we have counts for
6 papers
Time-dependent simulations of steady C-type shocks
S. Van Loo, I. Ashmore, P. Caselli +2
Using a time-dependent multifluid, magnetohydrodynamic code, we calculated the structure of steady perpendicular and oblique C-type shocks in dusty plasmas. We included relevant pr…
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…
Cold gas in the Intra Cluster Medium: implications for flow dynamics and powering optical nebulae
Edward Pope, Thomas Hartquist, Julian Pittard
We show that the mechanical energy injection rate generated as the intra-cluster medium (ICM) flows around cold clouds may be sufficient to power the optical and near infra-red emi…
The generation of optical emission-line filaments in galaxy clusters
Edward Pope, Julian Pittard, Thomas Hartquist +1
Recent data support the idea that the filaments observed in H_alpha emission near the centres of some galaxy clusters were shaped by bulk flows within their intracluster media. We…
Parametrization of C-shocks. Evolution of the Sputtering of Grains
I. Jimenez-Serra, P. Caselli, J. Martin-Pintado +1
Context: The detection of narrow SiO lines toward the young shocks of the L1448-mm outflow has been interpreted as a signature of the magnetic precursor of C-shocks. In contrast wi…
The Formation of Fragments at Corotation in Isothermal Protoplanetary Disks
Richard H. Durisen, Thomas W. Hartquist, Megan K. Pickett
Numerical hydrodynamics simulations have established that disks which are evolved under the condition of local isothermality will fragment into small dense clumps due to gravitatio…