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Comparison of s-Processing Occurring in a Low Mass AGB Star of Low Metallicity and the Results of s-Classical Analysis

Published online by Cambridge University Press:  12 April 2016

M. Busso ,
G. Picchio ,
R. Gallino ,
F. Kappeler  and
C.M. Raiteri
M. Busso
Affiliation:
Osservatorio Astronomico
G. Picchio
Affiliation:
Osservatorio Astronomico
R. Gallino
Affiliation:
Instituto Di Fisica
F. Kappeler
Affiliation:
Kernforschungszentrum
C.M. Raiteri
Affiliation:
International School for Advanced Studies

Extract

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We examine the results of s-Processlng occurring in a low mass star of low metallicity during the pulsed He-instability in AGB phases by comparing them with the s-Classical analysis. Neutron exposures are provided by the C13(Alpha, N)016 reaction, according to the mechanism suggested by Iben and Renzini (1983) for the formation in the interpulse phase of a small zone rich of C13 and its subsequent ingestion in the next pulse.

Type
3. Evolution of Peculiar Red Giant Stars
Information
International Astronomical Union Colloquium , Volume 106: Evolution of Peculiar Red Giant Stars , 1989 , pp. 237
Copyright
Copyright © Cambridge University Press 1989