Expanding the size of the simulation will allow the team to test an alternate theory for the emergence of galactic wind in disk galaxies like M82. (sciencedaily.com)
Furthermore, the team can zoom in on parts of the simulation to study phases and properties of galactic wind in isolation. (sciencedaily.com)
The observed CH + reveals dense shock waves, powered by hot, fast galactic winds originating inside the galaxies» star forming regions. (alma-telescope.jp)