A New Reaction Rate of the 27Al(p,γ)28Si Reaction Based on Indirect Low-energy Cross-section Measurements

The Mg–Al cycle is characteristic of the high-temperature ( T  ∼ 0.055 GK) H-burning of evolved stars and their nucleosynthesis. A proper comprehension of this reaction network can help in solving debated questions such as the occurrence of anticorrelation in Mg–Al abundances in globular clusters. R...

詳細記述

書誌詳細

出版年:	The Astrophysical Journal
主要な著者:	M. La Cognata, S. Palmerini, F. Dell’Agli, P. Ventura, P. Adsley, R. Alba, S. Cherubini, M. Costa, A. Di Pietro, P. Figuera, G. L. Guardo, M. Gulino, F. Hammache, M. La Commara, L. Lamia, D. Lattuada, C. Maiolino, M. Mazzocco, A. Oliva, R. G. Pizzone, P. M. Prajapati, G. G. Rapisarda, S. Romano, D. Santonocito, M. L. Sergi, R. Spartá, A. Tumino
フォーマット:	論文
言語:	英語
出版事項:	IOP Publishing 2025-01-01
主題:	Nuclear astrophysics Globular star clusters Isotopic abundances
オンライン･アクセス:	https://doi.org/10.3847/1538-4357/adb7e4