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- W2000728680 abstract "The visual absolute magnitudes of carbon stars are determined using double stars, carbon stars in clusters, and the Wilson-Bappu effect. Combining these magnitudes with previous results for carbon stars in the Large Magellanic Cloud and from radial-velocity and proper-motion studies, we obtain average visual absolute magnitudes for R stars of +0TM4, and for N-M3.5 to N-M6 stars of 1Φ5 to 3Ψ5 as a function of spectral type. The bolometric absolute magnitudes of R stars are close to those of Κ giants while the Ν stars are distinctly brighter than M giants, falling in luminosity class II." @default.
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- W2000728680 date "1968-10-01" @default.
- W2000728680 modified "2023-10-17" @default.
- W2000728680 title "The Absolute Magnitudes of Carbon Stars" @default.
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- W2000728680 doi "https://doi.org/10.1086/128694" @default.
- W2000728680 hasPublicationYear "1968" @default.
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