Spectral energy distributions of stars derived from Fourier transform spectrometry

Details Spectral energy distributions of stars derived from Fourier transform spectrometry Spectral energy distributions of stars derived from Fourier transform spectrometry

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apjs...34..101p&link_type=abstract

Astrophysical Journal Supplement Series, vol. 34, June 1977, p. 101-114. Research supported by the National Research Council of

Astronomy and Astrophysics

Astrophysics

45

Fourier Transformation, Light (Visible Radiation), Spectral Energy Distribution, Spectral Resolution, Spectrum Analysis, Stellar Spectrophotometry, Late Stars, Line Spectra, Spectral Bands, Stellar Luminosity, Stellar Spectra, Tables (Data)

Scientific paper

A birefringent Fourier spectrometer has been used to obtain spectrophotometry of 96 stars over the wavelength range from 3800 to 6800 A. The resolution (spectral purity) of these observations ranges from 12 A at 3800 A to 45 A at 6800 A. A total of 33 temperature- and/or luminosity-sensitive features were found. These features form a useful supplement to those strong lines and bands that are usually used for spectral classification at narrow-band resolution.

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