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arXiv · astro-ph/0203460

Radiation Driven Implosion of Molecular Cloud Cores

Olaf Kessel-Deynet·Andreas Burkert
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Abstract

We present the first three-dimensional calculations of Radiation Driven Implosion of Molecular Clouds including self-gravity and ionization. We discuss the effects of initial density perturbations on the dynamics of ionizing globules and show that the onset of gravitational collapse can be significantly delayed for a multiple of the implosion timescale. We demonstrate that Radiation Driven Implosion could be an efficient process for injecting disordered kinetic energy into molecular clouds in the vicinity of massive stars.

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Olaf Kessel-Deynet, Andreas Burkert. 2002-03-26. Radiation Driven Implosion of Molecular Cloud Cores. https://doi.org/10.1046/j.1365-8711.2003.05737.x

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