Multi-technique observations and modeling of protoplanetary disks

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

doi:10.1063/1.3099132

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 proceeding › Conference contribution

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 (US)
Title of host publication	AIP Conference Proceedings
Pages	401-404
Number of pages	4
Volume	1094
DOIs	https://doi.org/10.1063/1.3099132
State	Published - 2009
Externally published	Yes
Event	15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun - St. Andrews, United Kingdom Duration: Jul 21 2008 → Jul 25 2008

Other

Other	15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun
Country/Territory	United Kingdom
City	St. Andrews
Period	7/21/08 → 7/25/08

Keywords

Dust evolution
Molecular lines
Protoplanetary disk
Radiative transfert
Star formation

ASJC Scopus subject areas

Physics and Astronomy(all)

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10.1063/1.3099132

Cite this

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title = "Multi-technique observations and modeling of protoplanetary disks",

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.",

keywords = "Dust evolution, Molecular lines, Protoplanetary disk, Radiative transfert, Star formation",

author = "C. Pinte and F. M{\'e}nard and G. Duch{\^e}ne and J. Patience and C. Ceccarelli and G. Duvert",

year = "2009",

doi = "10.1063/1.3099132",

language = "English (US)",

volume = "1094",

pages = "401--404",

booktitle = "AIP Conference Proceedings",

note = "15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun ; Conference date: 21-07-2008 Through 25-07-2008",

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T1 - Multi-technique observations and modeling of protoplanetary disks

AU - Pinte, C.

AU - Ménard, F.

AU - Duchêne, G.

AU - Patience, J.

AU - Ceccarelli, C.

AU - Duvert, G.

PY - 2009

Y1 - 2009

N2 - 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.

AB - 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.

KW - Dust evolution

KW - Molecular lines

KW - Protoplanetary disk

KW - Radiative transfert

KW - Star formation

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U2 - 10.1063/1.3099132

DO - 10.1063/1.3099132

M3 - Conference contribution

VL - 1094

SP - 401

EP - 404

BT - AIP Conference Proceedings

T2 - 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun

Y2 - 21 July 2008 through 25 July 2008

ER -

Multi-technique observations and modeling of protoplanetary disks

Abstract

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Keywords

ASJC Scopus subject areas

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