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Reactions such as 25Al(p,γ)26Si are the key to understand the production of 26gAl and 26mAl in our galaxy. Experimental results could provide important constraints on nova nucleosynthesis and modelling where 26Al is believed to be produced. To achieve such measurements, high-intensity and high-purity radioactive beams are required. However, production targets at ISOL-type facilities such as ISAC...
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