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Infrared spectroscopy in astronomyThe use of infrared spectroscopy in astronomy has increased dramatically in the past ten years. The broad design considerations are discussed in terms of wavelength coverage and resolution. Three rough resolution ranges, lambda/Delta lambda of approximately 100, 1000 and 10,000, are identified in which various types of astronomical problems can be studied. Numerous existing systems are briefly discussed and references are given to more complete descriptions.
Document ID
19830032235
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Houck, J. R. (Cornell University Ithaca, NY, United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1981
Subject Category
Astronomy
Meeting Information
Meeting: Infrared astronomy - Scientific/military thrusts and instrumentation
Location: Washington, DC
Start Date: April 21, 1981
End Date: April 22, 1981
Accession Number
83A13453
Funding Number(s)
CONTRACT_GRANT: NGR-33-010-081
Distribution Limits
Public
Copyright
Other

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