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Paper: Models of the Infrared Spectral Energy Distribution of Embedded Super-Star Clusters
Volume: 322, The Formation and Evolution of Massive Young Star Clusters
Page: 541
Authors: Sauvage, M.; Vanzi, L.; Plante, S.
Abstract: We present radiation transfer models of the IR-mm spectral energy distribution of embedded super-star clusters observed in the dwarf galaxies NGC5253 and SBS 0335-052, one of the most metal-poor galaxy known. We show that the embedded cluster represent a very significant fraction of the current star formation activity and bolometric luminosity of their host, even if they are extremely compact compared to the size of their host.
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