Simulations from "Using Molecular Gas Observations to Guide Initial Conditions for Star Cluster Simulations"

<p>This dataset contains the simulation results&nbsp;from the article &quot;Using Molecular Gas Observations to Guide Initial Conditions for Star Cluster Simulations&quot; (submitted to MNRAS).</p> <p><br> The data is grouped by simulation and by particle type (gas, sinks and stars). Gas is uploaded with one snapshot per 0.05 Myr, sinks and stars with one snapshot per 0.01 Myr. The data is stored in AMUSE data format, which uses hdf5.</p>