Published September 9, 2021
| Version v1
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Yields from paper: ALUMINIUM-26 FROM MASSIVE BINARY STARS II. ROTATING SINGLE STARS UP TO CORE-COLLAPSE AND THEIR IMPACT ON THE EARLY SOLAR SYSTEM
Authors/Creators
- 1. Konkoly Observatory, University of Szeged
- 2. Konkoly Observatory
- 3. Konkoly Observatory, Monash University
- 4. E. A. Milne Centre for Astrophysics, Konkoly Observatory, NuGrid Collaboration, Joint Institute for Nuclear Astrophysics
- 5. Konkoly Observatory, Monash University, ELTE Eötvös Loránd University
Description
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 three files with the complete set
of yields from the models presented in this paper. YieldsNR.txt contains the yields for the
non-rotating models and Yields150.txt and Yields300.txt the yields for the models
rotating at an initial velocity of 150 and 300 km/s, respectively.
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Notes
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
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