Open clusters in a dispersing molecular cloud

Details Open clusters in a dispersing molecular cloud Open clusters in a dispersing molecular cloud

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008an....329.1053c&link_type=abstract

Astronomische Nachrichten, Vol.329, Issue , p.1053

Astronomy and Astrophysics

Astronomy

2

Open Clusters And Associations: General, Methods: N-Body Simulations

Scientific paper

Star clusters are formed in molecular clouds which are believed to be the birth places of most stars. From recent observational data, Lada & Lada (2003) estimated that only 4 to 7% of the proto-clusters have survived. A possible reason is the dispersion of molecular clouds by UV radiation, stellar winds or supernova explosions. We study the cloud dispersion in the embedded clusters by N-body simulations.

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