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Gas at the inner disk edge

Published online by Cambridge University Press:  01 May 2007

John S. Carr
John S. Carr*
Affiliation:
Naval Research Laboratory, Remote Sensing Division, Washington, DC 20375, USA email: carr@nrl.navy.mil
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Abstract

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Infrared molecular spectroscopy is a key tool for the observation of gas in the innermost region of disks around T Tauri stars. In this contribution, we examine how infrared spectroscopy of CO can be used to study the inner truncation region of disks around T Tauri stars. The inferred inner gas radii for T Tauri star disks are compared to the inner dust radii of disks, to the expectations of models for disk truncation, and to the orbital distribution of short-period extra-solar planets.

Keywords

Accretion disksprotoplanetary disksstars: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S243: Star-Disk Interaction in Young Stars , May 2007 , pp. 135 - 146
Copyright
Copyright © International Astronomical Union 2007

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