Sequential formation of massive stars and clusters at the periphery of H II regions

Details Sequential formation of massive stars and clusters at the periphery of H II regions Sequential formation of massive stars and clusters at the periphery of H II regions

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..322..375d&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 use multi-wavelength observations of two H II regions, Sh 104 and RCW
79, to discuss the `collect and collapse' process of massive-star
formation, triggered by the expansion of an H II region.

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