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

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

School of Physics and Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

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
Title of host publication	Cool Stars, Stellar Systems and the Sun
Editors	E Stempels
Place of Publication	MELVILLE
Publisher	American Institute of Physics
Pages	225-233
Number of pages	9
ISBN (Print)	978-0-7354-0627-8
Publication status	Published - 2009
Event	15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun - St Andrews, St Andrews, United Kingdom Duration: 21 Jul 2008 → 25 Jul 2008

Conference

Conference	15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun
Country/Territory	United Kingdom
City	St Andrews
Period	21/07/08 → 25/07/08

Cite this

@inproceedings{13ad5c737ca443759652ede00d29fe55,

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.",

author = "Peter Woitke and Bill Dent and Wing-Fai Thi 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",

year = "2009",

language = "English",

isbn = "978-0-7354-0627-8",

pages = "225--233",

editor = "E Stempels",

booktitle = "Cool Stars, Stellar Systems and the Sun",

publisher = "American Institute of Physics",

address = "United States",

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

}

Woitke, P, Dent, B, Thi, W-F, Sibthorpe, B, Rice, K, Williams, J, Sicilia-Aguilar, A, Brown, J, Kamp, I, Pascucci, I, Alexander, R & Roberge, A 2009, Gas Evolution in Protoplanetary Disks. in E Stempels (ed.), Cool Stars, Stellar Systems and the Sun. American Institute of Physics, MELVILLE, pp. 225-233, 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, St Andrews, United Kingdom, 21/07/08.

TY - GEN

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

Y1 - 2009

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.

M3 - Conference contribution

SN - 978-0-7354-0627-8

SP - 225

EP - 233

BT - Cool Stars, Stellar Systems and the Sun

A2 - Stempels, E

PB - American Institute of Physics

CY - MELVILLE

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

Conference

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