Stochastic Star Formation and Bubbles in the Large Magellanic Cloud
Abstract
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.
- Publication:
-
Structure and Evolution of the Magellanic Clouds
- Pub Date:
- September 1984
- DOI:
- 10.1017/S007418090003998X
- Bibcode:
- 1984IAUS..108...89F