3D hydrodynamic simulations of carbon burning in massive stars-Reference-Cited by-同舟云学术

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3D hydrodynamic simulations of carbon burning in massive stars

Published:2017-06-20 Issue:1 Volume:471 Page:279-300
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Cristini A.^ORCID,Meakin C.,Hirschi R.,Arnett D.,Georgy C.,Viallet M.,Walkington I.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/471/1/279/19371775/stx1535.pdf

Reference81 articles.

1. Low-temperature Rosseland opacities

2. A compilation of charged-particle induced thermonuclear reaction rates

3. Explosive Ignition of Carbon in Stars of Intermediate Mass

4. Oxgen-burning hydrodynamics. 1: Steady shell burning

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