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Interstellar Gas Dynamics

Published online by Cambridge University Press:  25 April 2016

M.E. Dixon
M.E. Dixon*
Affiliation:
Mount Stromlo Observatory, Australian National University, Canberra
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Extract

It is a well established observational result that young stars exhibit differences in chemical composition. The differences are comparatively large. For example, some stars have metal abundances as high as 3/2 solar-value while others have abundances as low as 1/2 solar-value. The result was obtained through spectroscopic and photoelectric studies of stars with ages of a few times 108 yr and indicates that the interstellar medium is chemically heterogeneous at the present epoch.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 3 , February 1968 , pp. 96
Copyright
Copyright © Astronomical Society of Australia 1968

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References

1 Eggen, O.J., R. Obs. Bulls, 82, E3 (1964).Google Scholar
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