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Fig. 11


Top: radial distribution of the gas and stellar mass density around Sgr B2(NE), Sgr B2(N), Sgr B2(M) and Sgr B2(S). Bottom: calculated star formation efficiency for Sgr B2(NE), Sgr B2(N), Sgr B2(M), and Sgr B2(S). The vertical dashed lines mark the extent of each star cluster. The same colors belong to the same clusters.

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