Sequential Formation of Massive Stars at the Periphery of H II Regions

Details Sequential Formation of Massive Stars at the Periphery of H II Regions Sequential Formation of Massive Stars at the Periphery of H II Regions

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..160d&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

Ism: H Ii Regions, Stars: Formation

Scientific paper

The ``collect and collapse'' model predicts that massive objects--stars or clusters--should form in the shocked neutral layer surrounding an expanding H II region when this layer becomes gravitationally unstable and fragments. We present several cases of H II regions and their associated clusters that seem to be good illustrations of this process of triggered star formation.

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