Multi-technique observations and modeling of protoplanetary disks

C. Pinte, F. Ménard, G. Duchêne, J. Patience, C. Ceccarelli, G. Duvert

Research output: Chapter in Book/Report/Conference proceedingConference PaperResearchpeer-review

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 languageEnglish
Title of host publicationAIP Conference Proceedings
Subtitle of host publication15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun; St. Andrews; United Kingdom; 21 July 2008 through 25 July 2008
Pages401-404
Number of pages4
Volume1094
DOIs
Publication statusPublished - 1 Jan 2009
Externally publishedYes
Event15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun - St. Andrews, United Kingdom
Duration: 21 Jul 200825 Jul 2008

Publication series

NameAIP Conference Proceedings
PublisherAIP Publishing
ISSN (Print)0094-243X

Conference

Conference15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun
CountryUnited Kingdom
CitySt. Andrews
Period21/07/0825/07/08

Keywords

  • Dust evolution
  • Molecular lines
  • Protoplanetary disk
  • Radiative transfert
  • Star formation

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