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High-spectral-resolution observations of the 7.7-micron feature in HD 44179Observations of the moon and HD 44179 were obtained in the wavelength range of 7.5-8.5 microns at a resolving power of approximately 800. The spectrum of the moon shows absorptions caused by telluric methane. Use of the moon as a calibrator is effective in removing these atmospheric lines. The spectrum of HD 44179 shows that the 7.7-micron emission feature does not break up into discrete, resolved emission features. Instead, it must be a broad, apparently continuous, emission feature.
Document ID
19820044655
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Russell, R. W.
(Cornell Univ. Ithaca, NY, United States)
Gull, G.
(Cornell Univ. Ithaca, NY, United States)
Beckwith, S.
(Cornell University Ithaca, NY, United States)
Evans, N. J., II
(Texas, University Austin, TX, United States)
Date Acquired
August 10, 2013
Publication Date
February 1, 1982
Publication Information
Publication: Astronomical Society of the Pacific
Subject Category
Astronomy
Accession Number
82A28190
Funding Number(s)
CONTRACT_GRANT: NSG-2412
CONTRACT_GRANT: NSF AST-79-20966
Distribution Limits
Public
Copyright
Other

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