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arXiv · 0805.0386

Disk Dispersal and Planet Formation Time Scales

Lynne A. Hillenbrand
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Abstract

Well before the existence of exo-solar systems was confirmed, it was accepted knowledge that most -- if not all -- stars possess circumstellar material during the first one-to-several million years of their pre-main sequence lives, and thus that they commonly have the potential to form planets. Here I summarize current understanding regarding the evolution of proto-planetary dust and gas disks, emphasizing the diversity in evolutionary paths.

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Lynne A. Hillenbrand. 2008-05-03. Disk Dispersal and Planet Formation Time Scales. https://doi.org/10.1088/0031-8949/2008/t130/014024

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