Stellar Feedback and the Evolution of Young Embedded Star Clusters

Details Stellar Feedback and the Evolution of Young Embedded Star Clusters Stellar Feedback and the Evolution of Young Embedded Star Clusters

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009rmxac..35...82w&link_type=abstract

XII Latin American IAU Regional Meeting (Eds. G. Magris, G. Bruzual, & L. Carigi) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Hii Regions, Ism: Clouds, Open Clusters And Associations: General, Stars: Formation, Stars: Luminosity Function, Mass Function, Stars: Winds, Outflows

Scientific paper

In this contribution we present the first results of an theoretical attempt to address the question of the evacuation time-scale but also the star-formation efficiency and the influence of feedback on the most-massive star in a star cluster. With the use of stellar evolution models, known descriptions for the evolution of an ionised sphere around a star and further models to describe stellar winds, the effects of young stellar populations of different sizes are studied.

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