ESP August 2010 by ESP Magazine - Issuu
PDF) Low-velocity shocks: Signatures of turbulent dissipation in diffuse irradiated gas
PDF) Effective viscosity from cloud-cloud collisions in three-dimensional global SPH simulations
PDF) The Dawes Review 9: The role of cold gas stripping on the star formation quenching of satellite galaxies
festi ENTIER 2014 DERN 7-01-2013 BIS:1-8/festi.qxd
PDF) An uncertainty principle for star formation - II. A new method for characterising the cloud-scale physics of star formation and feedback across cosmic history
PDF) Low-velocity shocks: Signatures of turbulent dissipation in diffuse irradiated gas
PDF) An uncertainty principle for star formation - II. A new method for characterising the cloud-scale physics of star formation and feedback across cosmic history
PDF) The Dawes Review 9: The role of cold gas stripping on the star formation quenching of satellite galaxies
PDF) The Dawes Review 9: The role of cold gas stripping on the star formation quenching of satellite galaxies
PDF) Effective viscosity from cloud-cloud collisions in three-dimensional global SPH simulations
PDF) Effective viscosity from cloud-cloud collisions in three-dimensional global SPH simulations
PDF) Effective viscosity from cloud-cloud collisions in three-dimensional global SPH simulations
ASIC Gazette
Rob Tissera & Nathan D'Amour - Bring The Lights Down - YouTube
Rob Tissera & Luvdup @ Ark, Leeds Uni, 6-5-95
PDF) Low-velocity shocks: Signatures of turbulent dissipation in diffuse irradiated gas
PDF) Low-velocity shocks: Signatures of turbulent dissipation in diffuse irradiated gas
PDF) The Dawes Review 9: The role of cold gas stripping on the star formation quenching of satellite galaxies
festi ENTIER 2014 DERN 7-01-2013 BIS:1-8/festi.qxd
festi ENTIER 2014 DERN 7-01-2013 BIS:1-8/festi.qxd
Rob Tissera & Nathan D'Amour - Bring The Lights Down - YouTube
PDF) An uncertainty principle for star formation - II. A new method for characterising the cloud-scale physics of star formation and feedback across cosmic history
