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Shock waves in an ideal gas with variable density, the radiative and conductive heat fluxes in the presence of gravitational force and magnetic field via the Lie group technique
On the dynamics and survival of fractal clouds in galactic winds
W E Banda-Barragán, F J Zertuche, C Federrath, et al. Monthly Notices of the Royal Astronomical Society 486(4) 4526 (2019) https://doi.org/10.1093/mnras/stz1040
Formation of filaments and dense cores during molecular clouds collision
Propagation of strong cylindrical shock wave in a self-gravitating rotational axisymmetric mixture of small solid particles and perfect gas with density varying exponentially
Cylindrical shock wave generated by a moving piston in a rotational axisymmetric non-ideal gas with conductive and radiative heat-fluxes in the presence of azimuthal magnetic field
Clustered supernovae drive powerful galactic winds after superbubble breakout
Drummond Fielding, Eliot Quataert and Davide Martizzi Monthly Notices of the Royal Astronomical Society 481(3) 3325 (2018) https://doi.org/10.1093/mnras/sty2466
3D numerical simulation of molecular clouds collision process
Filament formation in wind–cloud interactions– II. Clouds with turbulent density, velocity, and magnetic fields
W. E. Banda-Barragán, C. Federrath, R. M. Crocker and G. V. Bicknell Monthly Notices of the Royal Astronomical Society 473(3) 3454 (2018) https://doi.org/10.1093/mnras/stx2541
Modeling of density stratification and filamentous structure formation in molecular clouds after shock wave collision
Filament formation in wind–cloud interactions – I. Spherical clouds in uniform magnetic fields
W. E. Banda-Barragán, E. R. Parkin, C. Federrath, R. M. Crocker and G. V. Bicknell Monthly Notices of the Royal Astronomical Society 455(2) 1309 (2016) https://doi.org/10.1093/mnras/stv2405
Magnetogasdynamic spherical shock wave in a non-ideal gas under gravitational field with conductive and radiative heat fluxes
Chemical enrichment of the pre-solar cloud by supernova dust grains
Matthew D. Goodson, Ian Luebbers, Fabian Heitsch and Christopher C. Frazer Monthly Notices of the Royal Astronomical Society 462(3) 2777 (2016) https://doi.org/10.1093/mnras/stw1796
Model of turbulent destruction of molecular clouds
Evolution of M82-like starburst winds revisited: 3D radiative cooling hydrodynamical simulations
C. Melioli, E. M. de Gouveia Dal Pino and F. G. Geraissate Monthly Notices of the Royal Astronomical Society 430(4) 3235 (2013) https://doi.org/10.1093/mnras/stt126
THE COLLAPSE OF TURBULENT CORES AND RECONNECTION DIFFUSION
MHD turbulence-Star Formation Connection: from pc to kpc scales
E. M. de Gouveia Dal Pino, R. Santos-Lima, A. Lazarian, et al. Proceedings of the International Astronomical Union 6(S274) 333 (2010) https://doi.org/10.1017/S174392131100723X
Numerical heat conduction in hydrodynamical models of colliding hypersonic flows
Galactic outflows and the pollution of the galactic environment by supernovae
Elisabete M. de Gouveia Dal Pino, Claudio Melioli, Anibale D’Ercole, Fabrizzio Brighenti and Alex Raga Advances in Space Research 46(4) 485 (2010) https://doi.org/10.1016/j.asr.2009.06.022
Local star formation triggered by supernova shocks in magnetized diffuse neutral clouds
M. R. M. Leão, E. M. de Gouveia Dal Pino, D. Falceta-Gonçalves, C. Melioli and F. G. Geraissate Monthly Notices of the Royal Astronomical Society 394(1) 157 (2009) https://doi.org/10.1111/j.1365-2966.2008.14337.x
The turbulent destruction of clouds - I. Ak-ε treatment of turbulence in 2D models of adiabatic shock-cloud interactions
The Interaction between a Pulsed Astrophysical Jet and Small‐Scale Heterogeneous Media
Kristopher Yirak, Adam Frank, Andrew Cunningham and Sorin Mitran The Astrophysical Journal 672(2) 996 (2008) https://doi.org/10.1086/523955
Local star formation triggered by SN shocks in magnetized diffuse neutral clouds
M. R. M. Leão, E. M. de Gouveia Dal Pino, D. Falceta-Gonçalves, C. Melioli and F. G. Geraissate Proceedings of the International Astronomical Union 4(S259) 105 (2008) https://doi.org/10.1017/S1743921309030191
Hydrodynamical simulations of Galactic fountains – I. Evolution of single fountains
Three‐Dimensional Simulations of a Starburst‐driven Galactic Wind
Jackie L. Cooper, Geoffrey V. Bicknell, Ralph S. Sutherland and Joss Bland‐Hawthorn The Astrophysical Journal 674(1) 157 (2008) https://doi.org/10.1086/524918
On the Hydrodynamic Interaction of Shock Waves with Interstellar Clouds. II. The Effect of Smooth Cloud Boundaries on Cloud Destruction and Cloud Turbulence
Fumitaka Nakamura, Christopher F. McKee, Richard I. Klein and Robert T. Fisher The Astrophysical Journal Supplement Series 164(2) 477 (2006) https://doi.org/10.1086/501530
ISM gas removal from starburst galaxies and the premature death of star
clusters