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Thermal pulses; p-capture, alpha-capture, s-process nucleosynthesis; and convective mixing in a star of intermediate mass

Iben, I., Jr.·1975·The Astrophysical Journal

Abstract

Schwarzschild and Haerm (1967), and Sanders (1967) have suggested that the synthesis of elements by slow neutron capture on iron and on elements heavier than iron may take place in stars undergoing thermal pulses. The drawbacks of the various specific mechanisms that have been proposed by various investigators are pointed out, noting at the same time that all the mechanisms have one common feature - many repeated neutron bursts separated by long periods of quiescence - which seems to be a crucial element in obtaining a cosmic distribution of s-process elements. A scheme capable of producing repeated neutron bursts and bringing neutron-capture products to the surface is proposed for stars experiencing thermal pulses.

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Metadata

Authors
Iben, I., Jr.
Venue
The Astrophysical Journal
Published
1975-03
Volume
196
Pages
525
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W1644176225
Cited by
339
References
0
FWCI
11.29
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Thermal pulses; p-capture, alpha-capture, s-process nucleosynthesis; and convective mixing in a star of intermediate mass. https://app.cochat.ai/papers/10.1086/153433
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Iben, I., Jr. (1975). Thermal pulses; p-capture, alpha-capture, s-process nucleosynthesis; and convective mixing in a star of intermediate mass. The Astrophysical Journal. https://doi.org/10.1086/153433

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