Published August 2008
| Published
Journal Article
Open
Disk-dispersal and planet-formation timescales
- Creators
- Hillenbrand, Lynne A.
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.
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/T130Attached Files
Published - HILps08.pdf
Files
HILps08.pdf
Files
(224.7 kB)
| Name | Size | Download all |
|---|---|---|
|
md5:d2e2fbeee4dd46c73bd63e5a9db0f0f1
|
224.7 kB | Preview Download |
Additional details
- Eprint ID
- 11175
- Resolver ID
- CaltechAUTHORS:HILps08
- Created
-
2008-07-22Created from EPrint's datestamp field
- Updated
-
2022-07-12Created from EPrint's last_modified field