Fig. 11
YVSG/YBG distribution map for NGC 604 (left) and NGC 595 (right) obtained using DustEM code with a 4 Myr star cluster ISRF for NGC 604 and for NGC 595. The contours correspond to the continuum-subtracted Hα image at high resolution (6′′) and the numbers refer to the location of the expanding ionized gas shells observed by Yang et al. (1996) for NGC 604 and Lagrois & Joncas (2009) for NGC 595. Pixel size is 6′′.
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