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 contribution


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 (US)
Title of host publicationAIP Conference Proceedings
Number of pages4
StatePublished - 2009
Externally publishedYes
Event15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun - St. Andrews, United Kingdom
Duration: Jul 21 2008Jul 25 2008


Other15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun
Country/TerritoryUnited Kingdom
CitySt. Andrews


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

ASJC Scopus subject areas

  • General Physics and Astronomy


Dive into the research topics of 'Multi-technique observations and modeling of protoplanetary disks'. Together they form a unique fingerprint.

Cite this