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Southern Standards for the CMT1 T2 System

Published online by Cambridge University Press:  25 April 2016

M. S. Bessell  and
S. L. Williams
M. S. Bessell
Affiliation:
Mount Stromlo and Siding Spring Observatory, Australian National University
S. L. Williams
Affiliation:
Mount Stromlo and Siding Spring Observatory, Australian National University
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Extract

The K giants are the brightest stars in clusters of both intermediate (∽ 108 years) and old (∽ 109-10 years) age. They have strong metal lines and strong bands of CN and CH in the optical spectrum, and are the logical objects in which to measure the metal abundance of such stellar systems and trace the evolution of heavy elements in the universe.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 3 , Issue 1 , September 1976 , pp. 40 - 41
Copyright
Copyright © Astronomical Society of Australia 1976

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References

Bessell, M. S., Proc. Astron. Soc. Pac.. (in press) (1976).Google Scholar
Canterna, K., Astron. J., 81, 228 (1976).CrossRefGoogle Scholar
Cousins, A. W. J., Mem. R. Astron. Soc, 77, 223 (1973).Google Scholar
Cousins, A. W. J., Mom. Not. Astron. Soc. S. Africa, 33, 149 (1974).Google Scholar