NGC 604, structure and attenuation

Details NGC 604, structure and attenuation NGC 604, structure and attenuation

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..322...65m&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.

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Scientific paper

We have performed a multi-wavelength study of NGC 604, a young SOBA, using a combination of HST and ground-based data. The attenuation by dust experienced by the associated giant H II region is quite patchy, with some areas showing almost no signs of the presence of dust and others completely hidden from view in the optical. We have also detected the presence of the 2175 Å feature in one of the stars with moderate extinction.

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