Comparison of predicted and observed spectral energy distribution of K and M stars. I - Alpha Bootis

Details Comparison of predicted and observed spectral energy distribution of K and M stars. I - Alpha Bootis Comparison of predicted and observed spectral energy distribution of K and M stars. I - Alpha Bootis

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...235..138a&link_type=abstract

Astrophysical Journal, Part 1, vol. 235, Jan. 1, 1980, p. 138-145.

Astronomy and Astrophysics

Astrophysics

29

K Stars, Late Stars, M Stars, Spectral Energy Distribution, Stellar Atmospheres, Stellar Models, Stellar Spectrophotometry, Radiant Flux Density, Stellar Luminosity, Stellar Mass, Stellar Temperature

Scientific paper

The 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.

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