Abstract
Most of the studies on circumstellar disks are based on models that put an emphasis on fitting either SEDs or scattered light images or molecular emission maps. In this contribution, we present a more general approach which aims at interpreting the increasing amount of observational data in the framework of a single model, in order to obtain a more global picture and to better characterize both the dust population and the gas disk properties. The main objective of this general method is to couple the constraints from the gas- and dust-oriented studies to shed light on aspects of the disk structure that are cannot otherwise be studied in a coherent manner.
| Original language | English |
|---|---|
| Title of host publication | AIP Conference Proceedings |
| Subtitle of host publication | 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun; St. Andrews; United Kingdom; 21 July 2008 through 25 July 2008 |
| Pages | 401-404 |
| Number of pages | 4 |
| Volume | 1094 |
| DOIs | |
| Publication status | Published - 1 Jan 2009 |
| Externally published | Yes |
| Event | Cambridge Workshop on Cool Stars, Stellar Systems and the Sun 2008 - St. Andrews, United Kingdom Duration: 21 Jul 2008 → 25 Jul 2008 Conference number: 15th |
Publication series
| Name | AIP Conference Proceedings |
|---|---|
| Publisher | AIP Publishing |
| ISSN (Print) | 0094-243X |
Conference
| Conference | Cambridge Workshop on Cool Stars, Stellar Systems and the Sun 2008 |
|---|---|
| Country/Territory | United Kingdom |
| City | St. Andrews |
| Period | 21/07/08 → 25/07/08 |
Keywords
- Dust evolution
- Molecular lines
- Protoplanetary disk
- Radiative transfert
- Star formation
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