Young stellar aggregates embedded in expanding supershells

Details Young stellar aggregates embedded in expanding supershells Young stellar aggregates embedded in expanding supershells

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..393..279s&link_type=abstract

The seventh astrophysical conference: Star formation, near and far. AIP Conference Proceedings, Volume 393, pp. 279-282 (1997).

Astronomy and Astrophysics

Astrophysics

Stellar Clusters And Associations, Origin, Formation, Evolution, Age, And Star Formation, Star Formation

Scientific paper

Numerical N-body investigation of dynamical evolution of young stellar aggregate embedded into massive interstellar cloud is presented. We consider gravitational interaction of stars with unprocessed gas during cloud disruption and expanding envelope formation. This interaction leads to dynamical cooling of the stars and its comovement with the envelope. This effect can mimic of stimulated star formation in the supershell. The dynamical cooling also leads to gravitational bound cluster formation in spite of low star formation efficiency.

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