Spectral Analysis of the CS Star R CMi.

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概要

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• The wavelengths, intensities, and identifications of about 3, 700 lines in the spectrum of the CS star R CMi from 4180A to 6720A have been completed. Atomic lines are predominant in R CMi. The molecular bands observed in R CMi are not different but much weaker than in the cool carbon stars.

• 日本学士院の論文

著者

• UTSUMI Kazuhiko

  Faculty of Integrated Arts and Sciences, Hiroshima University

関連論文

• Spectral Analysis of the Cool BaII Star HD 121447.
• Spectral Analysis of the CS Star R CMi.

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