Multi-technique observations and modeling of protoplanetary disks

Details Multi-technique observations and modeling of protoplanetary disks Multi-technique observations and modeling of protoplanetary disks

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1094..401p&link_type=abstract

COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun.

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Circumstellar Shells, Clouds, And Expanding Envelopes, Circumstellar Masers, Star Formation, Radiative Transfer, Scattering

Scientific paper

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.

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