Spectrophotometry of carbon stars. I

Details Spectrophotometry of carbon stars. I Spectrophotometry of carbon stars. I

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985afz....23...99o&link_type=abstract

(Astrofizika, vol. 23, July-Aug. 1985, p. 99-109) Astrophysics (ISSN 0571-7132), vol. 23, no. 1, Jan. 1986, p. 432-438. Translat

Astronomy and Astrophysics

Astrophysics

3

Carbon Stars, Spectral Energy Distribution, Stellar Spectrophotometry, Variable Stars, Continuous Spectra, Line Spectra, Molecular Absorption, Swan Bands

Scientific paper

The results are given of the spectrophotometric investigation of 56 carbon stars in the spectral range from 4000 to 6800 A with resolution 3 A. The observed energy distributions of these stars are determined relative to the flux at the wavelength 5556 A; they are presented in the form of graphs. The energy distributions have been obtained for the first time for 35 stars. Variation in the line Ba II 4554 A has been found in the spectra of St. Cam, UU Aur, and RV Mon. Large changes have taken place in the spectra of RT UMa and SS Vir. It is noted that the spectra of carbon stars have a depression, this being situated in different spectral regions for individual groups of stars.

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