Massive star cluster formation - I. High star formation efficiency while resolving feedback of individual stars

Open Access

Fig. B.4.

Star formation efficiency over time for the fiducial M6 cloud with T_w = 300,000 K and $M_{feedback} \geq 20 M_{⊙}$ $M_{\mathrm{feedback}}\ge 20\rm\, M_\odot$ (cool winds), the M6 cloud with T_w = 5,000,000 K and $M_{feedback} \geq 20 M_{⊙}$ $M_{\mathrm{feedback}}\ge 20\rm\, M_\odot$ (hot winds), and the M6 cloud with T_w = 5,000,000 K and $M_{feedback} \geq 8 M_{⊙}$ $M_{\mathrm{feedback}}\ge 8\rm\, M_\odot$ (hot winds, $M_{fb} = 8 M_{⊙}$ $M_{\mathrm{fb}} = 8\rm\, M_\odot$ ).

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