Dense clumps survive in the vicinity of R136 in 30 Doradus

Open Access

Fig. 13

$M_{g a s}^{d u s t}$ $M_{gas}^{dust}$ plotted against the ratio $M_{g a s}^{d u s t} / M_{v i r}$ $M_{gas}^{dust}/M_{vir}$ . We include the ratios found by Bot et al. (2007) in the SMC (cyan), Herrera et al. (2013) in N11 (blue), and Milky Way values calculated in Bot et al. (2007) (green). The clumps are labeled according to their 0.88 mm continuum labels. The horizontal black line marks the $M_{g a s}^{d u s t} / M_{v i r} = 1$ $M_{gas}^{dust}/M_{vir}=1$ equality.

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