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Title:
Gas Evolution in Protoplanetary Disks
Authors:
Woitke, Peter; Dent, Bill; Thi, Wing-Fai; Sibthorpe, Bruce; Rice, Ken; Williams, Jonathan; Sicilia-Aguilar, Aurora; Brown, Joanna; Kamp, Inga; Pascucci, Ilaria; Alexander, Richard; Roberge, Aki
Affiliation:
AA(UK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK), AB(UK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK), AC(UK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK), AD(UK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK), AE(Institute for Astronomy, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK), AF(Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu HI 96822), AG(Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany), AH(Max-Planck-Institut för extraterrestrische Physik, Postfach 1312, 85741 Garching, Germany), AI(Kapteyn Astronomidcal Institute, Postbus 800, 9700 AV Groningen, The Netherlands), AJ(Steward Observatory, The University of Arizona, 933 N. Cherry Avenue, Tucson, AZ-85718, USA), AK(Sterrewacht Leiden, Universiteit Leiden, Niels Bohrweg 2, 2300 RA Leiden, The Netherlands), AL(NASA Goddard Space Flight Center, Code 667, Greenbelt, MD 20771, USA)
Publication:
COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. AIP Conference Proceedings, Volume 1094, pp. 225-233 (2009). (AIPC Homepage)
Publication Date:
02/2009
Origin:
AIP
PACS Keywords:
Planetary rings, Accretion and accretion disks, Solar wind plasma; sources of solar wind
DOI:
10.1063/1.3099095
Bibliographic Code:
2009AIPC.1094..225W

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 hydro-dynamical 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.
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