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Comparison of predicted and observed spectral energy distribution of K and M stars. I - Alpha BootisThe K2 IIIp star Alpha Bootis has been observed from the ground at 0.536 to 1.070 microns, and from an airplane at 1.21 to 3.90 microns. In the present paper, an absolute flux curve, constructed from these observations with an overall precision greater than + or - 2% in F-lambda, is compared with previous photometry and spectrometry.
Document ID
19800038024
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/157618
Authors
Augason, G. C. (NASA Ames Research Center Moffett Field, CA, United States)
Taylor, B. J. (NASA Ames Research Center Moffett Field, CA, United States)
Strecker, D. W. (NASA Ames Research Center Moffett Field, CA, United States)
Erickson, E. F. (NASA Ames Research Center Moffett Field, CA, United States)
Witteborn, F. C. (NASA Ames Research Center Moffett Field, Calif., United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1980
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Accession Number
80A22194
Distribution Limits
Public
Copyright
Other

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