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The Role of Stellar Feedback in Star Cluster Formation

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Table 2.1: Initial conditions, numerical parameters and modifications of the simu-lations in this paper: (1): Σtot,0: the initial average gas surface density in M⊙ pc−2.(2): R: the radius of the initial spherical gas cloud in pc
Figure 2.1: Surface density of gas (orange) and stars (blue) in our fiducial run withparametersright:sphere.star clusters have appeared.mass, at which point the gas is blown out of the system by feedback, evacuating the( M = 3 × 107M⊙ and R = 50 pc, project
Figure 2.4: Integrated SFE ϵ2.11, which gives parametersint of the 15 parameter survey simulations plotted againstvarious functions of the initial simulation parameters M (mass) and R (radius).The points with error bars, “H2011 GMCs”, represent the populat
Figure 2.A.1: Star formation histories of test runs with parameters Mto 200and = 107 M⊙ R = 50 pc
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