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High resolution spectroscopy with CSHELLThe NASA Infrared Telescope Facility Cryogenic Echelle Spectrograph (CSHELL) was designed to fill a need for high sensitivity, high resolution, long slit near-infrared spectroscopy. Scientific programs in the areas of comets, planetary atmospheres, young stellar objects, the interstellar medium, and galactic dynamics have been pursued with CSHELL and are described herein. The future of the instrument is also discussed.
Document ID
19950031368
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1007/BF00430182
Authors
Greene, T. P. (Univ. of Hawaii HI, US, United States)
Tokunaga, A. T. (Univ. of Hawaii HI, US, United States)
Carr, J. S. (Ohio State Univ. OH, US, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1994
Publication Information
Publication: Experimental Astronomy
Volume: 3
Issue: 1-4
ISSN: 0922-6435
Subject Category
Astronomy
Accession Number
95A62967
Distribution Limits
Public
Copyright
Other

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