Published April 1, 2013
| Published
Journal Article
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The HCN-Water Ratio in the Planet Formation Region of Disks
Abstract
We find a trend between the mid-infrared HCN/H_2O flux ratio and submillimeter disk mass among T Tauri stars in Taurus. While it may seem puzzling that the molecular emission properties of the inner disk (
Additional Information
© 2013 American Astronomical Society. Received 2012 September 26; accepted 2013 February 10; published 2013 March 15. This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Support for this work was provided by NASA. Basic research in infrared astrophysics at the Naval Research Laboratory is supported by 6.1 base funding. J.N. thanks Sharmila Dey for assistance with the data analysis.Attached Files
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Additional details
- Eprint ID
- 38259
- Resolver ID
- CaltechAUTHORS:20130503-101423988
- NASA/JPL/Caltech
- Created
-
2013-05-03Created from EPrint's datestamp field
- Updated
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2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences