The astrophysical S factor of 12C(<mml:math altimg="si1.gif" overflow="scroll" xmlns:xocs="http://www.elsevier.com/xml/xocs/dtd" xmlns:xs="http://www.w3.org/2001/XMLSchema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.elsevier.com/xml/ja/dtd" xmlns:ja="http://www.elsevier.com/xml/ja/dtd" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:tb="http://www.elsevier.com/xml/common/table/dtd" xmlns:sb="http://www.elsevier.com/xml/common/struct-bib/dtd" xmlns:ce="http://www.elsevier.com/xml/common/dtd" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:cals="http://www.elsevier.com/xml/common/cals/dtd"><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi></mml:math>)16O at stellar energy-Reference-Cited by-同舟云学术

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The astrophysical S factor of 12C(α,γ)16O at stellar energy

Published:2012-05 Issue:1 Volume:711 Page:35-40
ISSN:0370-2693
Container-title:Physics Letters B
language:en
Short-container-title:Physics Letters B

Author:

Schürmann D.,Gialanella L.,Kunz R.,Strieder F.

Funder

DFG

INFN

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics

Reference44 articles.

1. The12C(α, γ)16O Reaction Rate and the Evolution of Stars in the Mass Range 0.8 ≤ M/M⊙ ≤ 25

2. Evolution of Massive Stars Up to the End of Central Oxygen Burning

3. The Chemical Composition of White Dwarfs as a Test of Convective Efficiency during Core Helium Burning

4. White dwarf cooling sequences

5. Cauldrons in the Cosmos;Rolfs,1988

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