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Some Closing Thoughts

Published online by Cambridge University Press:  19 July 2016

H. M. Van Horn
H. M. Van Horn*
Affiliation:
Department of Physics and Astronomy University of Rochester Rochester, NY 14627-0011, USA

Extract

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I am very pleased to be the final speaker at this conference, for it gives me the pleasant opportunity to do several special things.

Type
Concluding Remarks
Information
Symposium - International Astronomical Union , Volume 145: Evolution of Stars: The Photospheric Abundance Connection , 1991 , pp. 461 - 469
Copyright
Copyright © Kluwer 1991 

References

Iben, I., and Tutukov, A. V. (1989) ‘Model Stars with Degenerate Dwarf Cores and Helium-Burning Shells: A Stationary-Burning Approximation’, Ap. J., 342, 430.Google Scholar
Sandage, A. (1987) ‘Summary - Population II Stars’ in IAU Coll. No. 95: The Second Conference on Faint Blue Stars , Philip, A. G. D., Hayes, D. S., and Liebert, J. W. (eds.), L. Davis Press, Schenectady, p. 469.Google Scholar
Vauclair, S., and Vauclair, G. (1982) ‘Element Segretation in Stellar Outer Layers’, Ann. Rev. Astron. Astrophys., 20, 37.CrossRefGoogle Scholar
Wheeler, J. C., Sneden, C., and Truran, J. W. (1989) ‘Abundance Ratios as a Function of Metallicity’ Ann. Rev. Astron. Astrophys., 27, 279.Google Scholar