| | 41 | |
| | 42 | Here we denote the number of sinks per run, as well as the frame they start forming. From this we determine what time in Myr they begin to form. Given a low shear angle and a weak magnetic field, we expect more sinks to form. |
| | 43 | |
| | 44 | See the following literature: |
| | 45 | |
| | 46 | * [http://adsabs.harvard.edu/abs/2004ApJ...611..399K] ''Embedding Lagrangian Sink Particles in Eulerian Grids'' by Krumholz, et al. |
| | 47 | * [http://adsabs.harvard.edu/abs/2010ApJ...713..269F] ''Modeling Collapse and Accretion in Turbulent Gas Clouds: Implementation and Comparison of Sink Particles in AMR and SPH'' by Federrath et al. |
| | 48 | |