Models of the infrared spectral energy distribution of embedded super-star clusters

Details Models of the infrared spectral energy distribution of embedded super-star clusters Models of the infrared spectral energy distribution of embedded super-star clusters

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..322..541s&link_type=abstract

The Formation and Evolution of Massive Young Star Clusters, ASP Conference Series, Vol. 322. Edited by H.J.G.L.M. Lamers, L.J.

Astronomy and Astrophysics

Astronomy

Scientific paper

We present radiation transfer models of the IR-mm spectral energy distribution of embedded super-star clusters observed in the dwarf galaxies NGC 5253 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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