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Two of the most Metal-deficient Stars

Published online by Cambridge University Press:  25 April 2016

M. S. Bessel
M. S. Bessel*
Affiliation:
Mount Stromlo and Siding Spring Observatory, Australian National University
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Extract

The metal content of stars (and galaxies) is of great interest as it relates to the theories of element formation, and through these to the history of our galaxy, the frequency of supernovae, the star formation rate and even the quasar rate. The kinematics and metallicity of stars have been correlated in a theory of formation of the galaxy by Eggen et al. (1962). Alternate theories (Unsold 1969) have also been proposed. Much work has gone into isolating individual metal deficient stars and determining their abundances, and also the abundances for stars in clusters.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 3 , Issue 2 , September 1977 , pp. 144 - 145
Copyright
Copyright © Astronomical Society of Australia 1977

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References

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