Other
Scientific paper
Sep 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pasp..105..905k&link_type=abstract
Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 105, no. 691, p. 905-910.
Other
51
Carbon Stars, H Beta Line, Red Giant Stars, Stellar Atmospheres, Stellar Spectra, Abundance, Astronomical Catalogs, G Stars, K Stars
Scientific paper
The spectral classification of the red carbon stars has been brought into the revised MK system by combining some of the features of the old R, N, and C classifications, as modified by Yamashita, and adding numerical abundance indices. The new types are intended to (1) define the population to which the star belongs, (2) allow quick interpolation between the detailed atmospheric analyses of individual stars, and (3) indicate the differences between carbon stars in different parts of our galaxy, and in other galaxies. It is the flexibility of the notation, allowing the incorporation of improved criteria, that should make the new system useful.
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