HIGHLIGHTS
- who: Frost-Schenk J. et al. from the of Physics, University of York, York , DD, UK have published the Article: The impact of 17Ou00a0+u00a0u03b1 reaction rate uncertainties on the s-process in rotating massive stars, in the Journal: (JOURNAL)
- what: From the current data, the authors determine n=14(5) keV. The only differences between the models shown in Fig 6 (left-hand panel) and the model shown by the solid red line in Fig 5 are the rates of 17 O(u03b1, n)20 Ne and 17 O(u03b1, u03b3 )21 Ne.
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