Experimental Determination of Widths of 21Ne Levels in the Region of Astrophysical Interest New 17O Reaction Rates and Impact on the Weak s Process

dc.article.end-page6en
dc.article.start-page1en
dc.citation.doi10.1103/PHYSREVLETT.132.182701en
dc.contributor.authorF. Hammacheen
dc.contributor.authorPhilip Adsleyen
dc.contributor.authorL. Lamiaen
dc.contributor.authorD.S. Harrouzen
dc.contributor.authorN. de Serevilleen
dc.contributor.authoral eten
dc.date.accessioned2024-09-16T09:53:34Z
dc.date.available2024-09-16T09:53:34Z
dc.facultyFACULTY OF SCIENCEen
dc.identifier.citationWOSen
dc.identifier.issn0031-9007en
dc.identifier.urihttps://hdl.handle.net/10539/40794
dc.journal.titleExperimental Determination of Widths of 21Ne Levels in the Region of Astrophysical Interest New 17O Reaction Rates and Impact on the Weak s Processen
dc.journal.volume132en
dc.publisherAMER PHYSICAL SOCen
dc.titleExperimental Determination of Widths of 21Ne Levels in the Region of Astrophysical Interest New 17O Reaction Rates and Impact on the Weak s Processen
dc.typeJournal Articleen
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