================================================================================ 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. ================================================================================ 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. ================================================================================

This work is supported by the ERC via CoG-2016 RADIOSTAR (Grant Agreement 724560). We also acknowledge support from "ChETEC" COST Action(CA16117), supported by COST (European Cooperation in Science andTechnology). MP acknowledges significant support to NuGrid from STFC (through the University of Hull's Consolidated Grant ST/R000840/1), from the National Science Foundation (NSF, USA) under grant No. PHY-1430152 (JINA Center for the Evolution of the Elements) and from the "Lendulet-2014" Program of the Hungarian Academy of Sciences (Hungary). MP thanks for the support from the US IReNA Accelnet network