Multi-technique observations and modeling of protoplanetary disks

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

Research output: Contribution to journalConference article

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 (US)
Pages (from-to)401-404
Number of pages4
JournalAIP Conference Proceedings
Volume1094
DOIs
StatePublished - Jan 1 2009
Externally publishedYes
Event15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun - St. Andrews, United Kingdom
Duration: Jul 21 2008Jul 25 2008

Keywords

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

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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  • Cite this

    Pinte, C., Ménard, F., Duchêne, G., Patience, J., Ceccarelli, C., & Duvert, G. (2009). Multi-technique observations and modeling of protoplanetary disks. AIP Conference Proceedings, 1094, 401-404. https://doi.org/10.1063/1.3099132