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Scanner observations of selected cool starsPhotoelectric spectral scans at 30-A resolution of 9 dwarfs, 10 giants and 6 supergiants with spectral types GO to M5 were presented. All stars were observed every 4 A from wavelength 3300 to wavelength 7000. Absorption features at this resolution coincide with: strong atomic lines of Fe 1,11, Ca 1,11, Mg 1, and Na 1; vibrational bands of the electronic transitions of TiO, MgH, CaH, SiH, AlH, Cn, Ch, C2, OH, and NH. The dependence of the wavelength 3740 Fe 1 blend and the wavelength 3440 depression on temperature is discussed.
Document ID
19740019235
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Fay, T. D., Jr.
(Alabama Univ. University, United States)
Stein, W. L.
(Indiana Univ. Bloomington, IN, United States)
Warren, W. H., Jr.
(Indiana Univ. Bloomington, IN, United States)
Date Acquired
September 3, 2013
Publication Date
March 27, 1974
Subject Category
Space Sciences
Report/Patent Number
NASA-CR-138777
Accession Number
74N27348
Funding Number(s)
CONTRACT_GRANT: NGL-15-003-002
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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