Gas evolution in protoplanetary disks

Peter Woitke; Bill Dent; Wing Fai Thi; Bruce Sibthorpe; Ken Rice; Jonathan Williams; Aurora Sicilia-Aguilar; Joanna Brown; Inga Kamp; Ilaria Pascucci; Richard Alexander; Aki Roberge

doi:10.1063/1.3099095

Gas evolution in protoplanetary disks

Peter Woitke, Bill Dent, Wing Fai Thi, Bruce Sibthorpe, Ken Rice, Jonathan Williams, Aurora Sicilia-Aguilar, Joanna Brown, Inga Kamp, Ilaria Pascucci, Richard Alexander, Aki Roberge

Physics

Research output: Contribution to journal › Conference article › peer-review

2 Citations (Scopus)

Abstract

This article summarizes a Splinter Session at the Cool Stars XV conference in St. Andrews with 3 review and 4 contributed talks. The speakers have discussed various approaches to understand the structure and evolution of the gas component in protoplanetary disks. These ranged from observational spectroscopy in the UV, infrared and millimeter, through to chemical and hydrodynamical models. The focus was on disks around low-mass stars, ranging from classical T Tauri stars to transitional disks and debris disks. Emphasis was put on water and organic molecules, the relation to planet formation, and the formation of holes and gaps in the inner regions.

Original language	English
Pages (from-to)	225-233
Number of pages	9
Journal	AIP Conference Proceedings
Volume	1094
DOIs	https://doi.org/10.1063/1.3099095
Publication status	Published - 25 Feb 2009
Event	15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun - St. Andrews, United Kingdom Duration: 21 Jul 2008 → 25 Jul 2008

Keywords

Accretion and accretion disks
And grain processes
Atomic
Chemical
Debris disks
Infrared excess
Mass loss and stellar winds
Molecular
Origin and evolution
Protoplanetary disk
Protostars
Solar system

ASJC Scopus subject areas

General Physics and Astronomy

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10.1063/1.3099095

Cite this

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title = "Gas evolution in protoplanetary disks",

abstract = "This article summarizes a Splinter Session at the Cool Stars XV conference in St. Andrews with 3 review and 4 contributed talks. The speakers have discussed various approaches to understand the structure and evolution of the gas component in protoplanetary disks. These ranged from observational spectroscopy in the UV, infrared and millimeter, through to chemical and hydrodynamical models. The focus was on disks around low-mass stars, ranging from classical T Tauri stars to transitional disks and debris disks. Emphasis was put on water and organic molecules, the relation to planet formation, and the formation of holes and gaps in the inner regions.",

keywords = "Accretion and accretion disks, And grain processes, Atomic, Chemical, Debris disks, Infrared excess, Mass loss and stellar winds, Molecular, Origin and evolution, Protoplanetary disk, Protostars, Solar system",

author = "Peter Woitke and Bill Dent and Thi, {Wing Fai} and Bruce Sibthorpe and Ken Rice and Jonathan Williams and Aurora Sicilia-Aguilar and Joanna Brown and Inga Kamp and Ilaria Pascucci and Richard Alexander and Aki Roberge",

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T1 - Gas evolution in protoplanetary disks

AU - Woitke, Peter

AU - Dent, Bill

AU - Thi, Wing Fai

AU - Sibthorpe, Bruce

AU - Rice, Ken

AU - Williams, Jonathan

AU - Sicilia-Aguilar, Aurora

AU - Brown, Joanna

AU - Kamp, Inga

AU - Pascucci, Ilaria

AU - Alexander, Richard

AU - Roberge, Aki

PY - 2009/2/25

Y1 - 2009/2/25

N2 - This article summarizes a Splinter Session at the Cool Stars XV conference in St. Andrews with 3 review and 4 contributed talks. The speakers have discussed various approaches to understand the structure and evolution of the gas component in protoplanetary disks. These ranged from observational spectroscopy in the UV, infrared and millimeter, through to chemical and hydrodynamical models. The focus was on disks around low-mass stars, ranging from classical T Tauri stars to transitional disks and debris disks. Emphasis was put on water and organic molecules, the relation to planet formation, and the formation of holes and gaps in the inner regions.

AB - This article summarizes a Splinter Session at the Cool Stars XV conference in St. Andrews with 3 review and 4 contributed talks. The speakers have discussed various approaches to understand the structure and evolution of the gas component in protoplanetary disks. These ranged from observational spectroscopy in the UV, infrared and millimeter, through to chemical and hydrodynamical models. The focus was on disks around low-mass stars, ranging from classical T Tauri stars to transitional disks and debris disks. Emphasis was put on water and organic molecules, the relation to planet formation, and the formation of holes and gaps in the inner regions.

KW - Accretion and accretion disks

KW - And grain processes

KW - Atomic

KW - Chemical

KW - Debris disks

KW - Infrared excess

KW - Mass loss and stellar winds

KW - Molecular

KW - Origin and evolution

KW - Protoplanetary disk

KW - Protostars

KW - Solar system

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U2 - 10.1063/1.3099095

DO - 10.1063/1.3099095

M3 - Conference article

AN - SCOPUS:64849088158

SN - 0094-243X

VL - 1094

SP - 225

EP - 233

JO - AIP Conference Proceedings

JF - AIP Conference Proceedings

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

Y2 - 21 July 2008 through 25 July 2008

ER -

Gas evolution in protoplanetary disks

Abstract

Keywords

ASJC Scopus subject areas

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