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NSR database version of May 10, 2024.

Search: Author = S.M.Reddy

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2024NE03      Astrophys.J. 964, 151 (2024)

N.D.Nevill, P.A.Bland, D.W.Saxey, W.D.A.Rickard, P.Guagliardo, N.E.Timms, L.V.Forman, L.Daly, S.M.Reddy

Atomic-scale Element and Isotopic Investigation of ²⁵Mg-rich Stardust from an H-burning Supernova

ATOMIC MASSES ²⁵Mg; analyzed available data; deduced isotopic compositions challenge current stellar models, with modeling of magnesium, silicon, and oxygen showing a closest match to formation in a supernova (SN) where hydrogen ingestion occurred in the pre-SN phase.

doi: 10.3847/1538-4357/ad2996
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