Inlists for paper: ALUMINIUM-26 FROM MASSIVE BINARY STARS II. ROTATING SINGLE STARS UP TO CORE-COLLAPSE AND THEIR IMPACT ON THE EARLY SOLAR SYSTEM
- 1. Konkoly Observatory, University of Szeged
- 2. Konkoly Observatory
- 3. Konkoly Observatory, Monash University
- 4. E. A. Milne Centre for Astrophysics,m Konkoly Observatory, NuGrid Collaboration, Joint Institute for Nuclear Astrophysics
- 5. Konkoly Observatory, Monash University, ELTE Eötvös Loránd University
Description
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Title: Aluminium-26 From Massive Binary Stars II: ROTATING SINGLE STARS UP TO CORE-COLLAPSE AND THEIR IMPACT ON THE EARLY SOLAR SYSTEM
Authors: Brinkman H.E., den Hartogh J. W., Doherty C.L., Pignatari M., Lugaro M.
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Description of contents: A .tar.gz package containing the input files for the
MESA simulations of massive (10 {<=} M*(solmass) {<=} 80) non-rotating and rotating,
single solar metallicity (Z=0.014). The files are in
the subdirectories /BlancoNR and /BlancoRotating. The nuclear network
used is also given, RadioSupernova.net
There are 4 basic files. The "inlist" file is the master inlist that MESA
reads when it starts. It reads the "_starjob", "_controls", and
"_pgstar" inlist files. For the single stars, subdirectory /Single, only one
set is needed. For both the rotating and the non-rotating set the run_star_extras.f is given as well.
System requirements: The MESA stellar evolution code. Version 10398 was used
for these input files.
Additional comments: See section 2 for full details of the simulations.
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Notes
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