Common Occurrence of Explosive Hydrogen Burning in Type II Supernovae
Nan Liu, Thomas Stephan, Patrick Boehnke, Larry R. Nittler, Bradley S., Meyer, Conel M. O'D. Alexander, Andrew M. Davis, Reto Trappitsch, Michael J., Pellin

TL;DR
This study presents isotopic evidence from presolar grains indicating that explosive hydrogen burning is a common process in the outer zones of Type II supernovae, contributing to our understanding of stellar nucleosynthesis.
Contribution
It provides new isotopic data linking presolar grains to supernova processes and demonstrates that explosive H burning occurs frequently in outer supernova zones.
Findings
AB1 grains show s-process isotopic compositions linked to supernovae.
Explosive H burning occurs in multiple zones of supernova progenitors.
Isotopic evidence supports frequent explosive H burning in Type II supernovae.
Abstract
We report Mo isotopic data for 16 15N-rich presolar SiC grains of type AB (14N/15N<solar, AB1) and their correlated Sr and Ba isotope ratios when available. Eight of the 16 AB1 grains show s-process Mo isotopic compositions, together with s-process Ba and/or Sr isotopic compositions. We found that a higher percentage of AB1 grains show anomalous isotopic compositions than that of AB2 grains (14N/15N>solar), thus providing further support to the division of the two AB subgroups recently proposed by Liu et al. (2017a), who showed that AB1 grains most likely originated from Type II supernovae (SNe) with explosive H burning. Comparison of the Sr, Mo, and Ba isotopic compositions of the AB1 grains with SN model predictions indicates that the s-process isotopic compositions of AB1 grains resulted from neutron-capture processes occurring during the progenitor massive stars' pre-SN evolution…
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