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Some observable indicators of s-process environments?

Published online by Cambridge University Press:  04 August 2017

Keith H. Despain
Keith H. Despain*
Affiliation:
Los Alamos National Laboratory

Abstract

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By definition, the chemically peculiar stars have element abundances that are non-solar. Many of these stars show peculiarities in s-process elements. This paper discusses observable indicators of the neutron environment for the s-process in these stars.

Type
I. EVOLUTION OF LOW AND INTERMEDIATE MASS STARS OBSERVATIONS AND MODELS
Information
Symposium - International Astronomical Union , Volume 105: Observational Tests of the Stellar Evolution Theory , 1984 , pp. 195 - 198
Copyright
Copyright © Reidel 1984 

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