High star formation rates as the origin of turbulence in early and modern disk galaxies
Supercomputer simulation of the formation of a disc galaxy similar to our own Milky Way. The calculation follows the dynamics of gas, stars and the cosmic dark matter from the Big Bang to the present day, and enables astronomers to visualise the turbulent nature of gas dynamics in both the ancient and present day Universe.
Any use of these visualisations must be credited:
Simulation by Rob Crain (Swinburne) and the Virgo Consortium
Visualisation by Rob Crain (Swinburne) and Jim Geach (McGill).
To download high resolutions versions, right click on the links below and choose "Save As":
|Windows Media||103 MB|