The density variance-Mach number relation in isothermal and non-isothermal adiabatic turbulence
The density variance-Mach number relation of the turbulent interstellar medium is relevant for theoretical models of the star formation rate, efficiency, and the initial mass function of stars. Here we use high-resolution hydrodynamical simulations with grid resolutions of up to 10243 cells to model compressible turbulence in a regime similar to the observed interstellar medium. We use FYRIS ALPHA, a shock-capturing code employing a high-order Godunov scheme to track large density variations...[Show more]
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|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Nolan_The_density_variance-Mach_2015.pdf||5.64 MB||Adobe PDF||Request a copy|
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