Stochastic Star Formation and Bubbles in the Large Magellanic Cloud

Details Stochastic Star Formation and Bubbles in the Large Magellanic Cloud Stochastic Star Formation and Bubbles in the Large Magellanic Cloud

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108...89f&link_type=abstract

Structure and Evolution of the Magellanic Clouds, Proceedings of IAU Symposium No. 108, held 5-8 September 1983 in Tübingen, Wes

Physics

1

Scientific paper

In the LMC ring nebulae or shell structures are often associated with OB
associations or WR-stars. This note discusses the bubble formation
process as a consequence of self-propagating stochastic star formation.

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