Curve-of-growth analysis of a red giant in the globular cluster M13

Details Curve-of-growth analysis of a red giant in the globular cluster M13 Curve-of-growth analysis of a red giant in the globular cluster M13

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.187..269g&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 187, Apr. 1979, p. 269-276. Research supported by the Science Research

Astronomy and Astrophysics

Astronomy

5

Abundance, Globular Clusters, Metallic Stars, Red Giant Stars, Stellar Evolution, Stellar Spectrophotometry, Rayleigh Scattering, Spectrograms, Stellar Spectra, Variable Stars

Scientific paper

A Coude spectrogram of a red giant (L973) in the globular cluster M13 is
analyzed with respect to Alpha Boo by the differential curve-of-growth
technique. The overall metal abundance is found to be approximately
one-tenth that of Alpha Boo, or one-fortieth that of the sun.

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