Journal ArticleDOI
Thermonuclear reaction rates V
TLDR
In this paper, the reaction rates of astrophysically important thermonuclear reactions involving low-mass nuclei were analyzed for the temperature range 106 ⩽ T ⌽ 1010 K.About:
This article is published in Atomic Data and Nuclear Data Tables.The article was published on 1988-11-01. It has received 1305 citations till now.read more
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Modules for Experiments in Stellar Astrophysics (MESA)
Bill Paxton,Lars Bildsten,Aaron Dotter,Aaron Dotter,Falk Herwig,Pierre Lesaffre,Francis Timmes +6 more
TL;DR: Modules for Experiments in Stellar Astrophysics (MESA) as mentioned in this paper is a suite of open source, robust, efficient, thread-safe libraries for a wide range of applications in computational stellar astrophysics.
Journal ArticleDOI
parsec: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code
Alessandro Bressan,Paola Marigo,Léo Girardi,Bernardo Salasnich,Claudia Dal Cero,Stefano Rubele,Ambra Nanni +6 more
TL;DR: In this article, the authors present an updated version of the AESOPUS code used to compute stellar evolutionary tracks in Padova, which is the result of a thorough revision of put physics, together with the inclusion of the pre-main sequence phase.
Journal ArticleDOI
PARSEC: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code
Alessandro Bressan,Paola Marigo,Léo Girardi,Bernardo Salasnich,C. Dal Cero,S. Rubele,Ambra Nanni +6 more
TL;DR: In this work, extended sets of stellar evolutionary models for various initial chemical compositions are presented, while other set s with different metallicities and/or different distributions of heavy elements are being computed.
Journal ArticleDOI
Flash: An adaptive mesh hydrodynamics code for modeling astrophysical thermonuclear flashes
B. Fryxell,K. Olson,Paul M. Ricker,Francis Timmes,Michael Zingale,D. Q. Lamb,Peter MacNeice,Robert Rosner,James W. Truran,Henry M. Tufo +9 more
TL;DR: The first version of a new-generation simulation code, FLASH, solves the fully compressible, reactive hydrodynamic equations and allows for the use of adaptive mesh refinement and contains state-of-the-art modules for the equations of state and thermonuclear reaction networks.
Journal ArticleDOI
The evolution and explosion of massive stars
TL;DR: In this article, the authors examined the current understanding of the lives and deaths of massive stars, with special attention to the relevant nuclear and stellar physics, and focused on their post-helium-burning evolution.
References
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Journal ArticleDOI
The 1983 atomic mass evaluation: (I). Atomic mass table
A.H. Wapstra,Georges Audi +1 more
TL;DR: In this article, a table is given to replace the 1977 atomic mass table and the differences from the earlier tables are briefly discussed and information is given of interest for users of this table.
Journal ArticleDOI
Thermonuclear reaction rates. II
TL;DR: In this paper, a review of the available experimental data on cross sections for the nuclear interactions of neutrons, protons, and alpha particles with a number of light and intermediate-mass nuclei is presented.
Journal ArticleDOI
Stellar weak interaction rates for intermediate-mass nuclei. IV - Interpolation procedures for rapidly varying lepton capture rates using effective log (ft)-values
TL;DR: In this paper, simple expressions for continuum electron and positron capture phase space factors and the associated neutrino energy loss integrals are presented in terms of standard Fermi integrals.
Journal ArticleDOI
Stellar weak interaction rates for intermediate mass nuclei. III. Rate tables for the free nucleons and nuclei with A = 21 TO A = 60
TL;DR: In this paper, the stellar electron and positron emission rates and neutrino energy loss rates for free nucleons and 226 nuclei with masses between A = 21 and 60 were calculated in tabular form on an abbreviated temperature and density grid.
Journal ArticleDOI
Tables of thermonuclear reaction rates for low-mass nuclei (1 ⩽ Z ⩽ 14)
Georgeanne R. Caughlan,Georgeanne R. Caughlan,William A. Fowler,William A. Fowler,Michael J. Harris,Michael J. Harris,Barbara A. Zimmerman,Barbara A. Zimmerman +7 more
TL;DR: In this paper, the numerical values of the thermonuclear reaction rates for astrophysically important reactions involving low-mass nuclei were tabulated for the temperature range 10/sup 6/< or =T < or =10/sup 10/ degrees Kelvin.
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