Hillenbrand, Lynne A. (2008) Disk-dispersal and planet-formation timescales. Physica Scripta, T130 . Art. No. 014024. ISSN 0031-8949. doi:10.1088/0031-8949/2008/T130/014024. https://resolver.caltech.edu/CaltechAUTHORS:HILps08
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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 these systems commonly have the potential to form planets. Here, I summarize current understanding regarding the evolution of protoplanetary disks.
| Item Type: | Article | |||||||||
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| Additional Information: | © 2008 The Royal Swedish Academy of Sciences. Received 11 March 2008, accepted for publication 14 March 2008. Published 16 July 2008. Print publication: Issue T130 (August 2008). Special issue: Nobel Symposium 135: Physics of Planetary Systems (18–22 June 2007, Lidingö, Stockholm, Sweden). Physica Scripta T130 http://www.iop.org/EJ/toc/1402-4896/2008/T130 | |||||||||
| DOI: | 10.1088/0031-8949/2008/T130/014024 | |||||||||
| Record Number: | CaltechAUTHORS:HILps08 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:HILps08 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 11175 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | Archive Administrator | |||||||||
| Deposited On: | 22 Jul 2008 02:59 | |||||||||
| Last Modified: | 12 Jul 2022 19:41 |
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