Abstract
Multiwavelength studies of evolved protoplanetary disks around solar-type and low-mass stars reveal a general trend of changes in the IR excesses, accretion rates, and silicate features, suggesting grain growth/settling, photoevaporation, and maybe the formation of planetesimals and planets. Nevertheless within the average-behavior picture of disk evolution, we observe strong variations between individuals, that may be related to different initial conditions, different environments, and the presence of companions.
| Original language | English |
|---|---|
| Title of host publication | COOL STARS, STELLAR SYSTEMS AND THE SUN |
| Subtitle of host publication | Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun |
| Editors | Michael Zeilik, David M. Gibson |
| Publisher | AIP Publishing |
| Pages | 23-28 |
| Number of pages | 6 |
| Volume | 1094 |
| ISBN (Print) | 9780735406278 |
| DOIs | |
| Publication status | Published - 16 Feb 2009 |
| Event | Cool Stars, Stellar Systems and the Sun: proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun - University of St Andrews, St. Andrews, United Kingdom Duration: 21 Jul 2008 → 25 Jul 2008 http://star-www.st-andrews.ac.uk/coolstars15/index.php?content=main |
Publication series
| Name | AIP Conference Proceedings |
|---|
Conference
| Conference | Cool Stars, Stellar Systems and the Sun |
|---|---|
| Country/Territory | United Kingdom |
| City | St. Andrews |
| Period | 21/07/08 → 25/07/08 |
| Internet address |
Keywords
- Stars: Formation Planetary systems: Protoplanetary disks Accretion disks T-TAURI STARS INTERSTELLAR SILICATE MINERALOGY SPITZER-SPACE-TELESCOPE ACCRETION DUST PLANET PHOTOEVAPORATION GROWTH GRAINS MODELS
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