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arXiv · astro-ph/9905167

Superbubble evolution including the star-forming clouds: Is it possible to reconcile LMC observations with model predictions?

S. Silich·J. Franco
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Abstract

Here we present a possible solution to the apparent discrepancy between the observed properties of LMC bubbles and the standard, constant density bubble model. A two-dimensional model of a wind-driven bubble expanding from a flattened giant molecular cloud is examined. We conclude that the expansion velocities derived from spherically symmetric models are not always applicable to elongated young bubbles seen almost face-on due to the LMC orientation. In addition, an observational test to differentiate between spherical and elongated bubbles seen face-on is discussed.

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S. Silich, J. Franco. 1999-05-13. Superbubble evolution including the star-forming clouds: Is it possible to reconcile LMC observations with model predictions?. https://doi.org/10.1086/307694

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