Chemical Inhomogeneities among Giant Stars in NGC 3201

Details Chemical Inhomogeneities among Giant Stars in NGC 3201 Chemical Inhomogeneities among Giant Stars in NGC 3201

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jkas...21...67c&link_type=abstract

Journal of the Korean Astronomical Society, vol. 21, p. 67-77

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Nine giant star's spectra in NGC 3201 were obtained using the image tube
in Sutherland. From the analysis of these spectra we found the increase
of Ca I and CH abundances with decreasing the radial distance, but CN,
Ca II and Fe abundances do not show this. Dependence of calculated
parameters seems to exist among CN, Ca I, Ca II and CH abundances.

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