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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 

References

Burbidge, EM and Burbidge, GR 1957, ApJ , 126, 357. (BB) Google Scholar
Burbidge, FM, Burbidge, GR, Fowler, WA, and Hoyle, F 1957, RMP , 29, 547.Google Scholar
Butcher, HR 1976, ApJ , 210, 489.Google Scholar
Cameron, AGW 1955, ApJ , 121, 144.CrossRefGoogle Scholar
Clayton, D, Fowler, W, Hull, T, and Zimmerman, B 1961, Ann Phys , 12, 331.CrossRefGoogle Scholar
Cosner, KR 1982, PhD thesis, Univ. of Ill.Google Scholar
Cowan, JJ, and Rose, WK 1977, ApJ , 212, 149.Google Scholar
Cowley, CR, 1968 ApJ , 153, 169. (C) Google Scholar
Cowley, CR, and Downs, PL 1980, ApJ , 236, 648. (CD) Google Scholar
Danziger, I 1965, MNRAS , 131, 51. (D) Google Scholar
Despain, KH 1977, ApJ 212 , 774.Google Scholar
Iben, I 1975, ApJ , 196, 549 Google Scholar
Langer, G, Kraft, R, and Anderson, K 1974, ApJ , 189, 509. (LKA) Google Scholar
Scalo, J. and Miller, G 1981, ApJ, 246, 251.Google Scholar
Sneden, C, and Bond, H 1976, ApJ , 204, 810. (SB) Google Scholar
Tech, JL 1971, NBS Monograph 119. (T).Google Scholar
Wallerstein, G, and Greenstein, J 1964, ApJ , 169, 1163. (WG) CrossRefGoogle Scholar
Warner, B 1965, MNRAS, 129, 263. (W) Google Scholar