New constraints for supernova models from presolar silicon carbide X grains with very high 26Al/27Al ratios
We report C, N, Mg-Al, Si, and S isotope data of six 1-3 μm-sized SiC grains of Type X from the Murchison CM2 chondrite, believed to have formed in the ejecta of core-collapse supernova (CCSN) explosions. Their C, N, and Si isotopic compositions are fully compatible with previously studied X grains....
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| Hauptverfasser: | , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2023 February 1
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| In: |
The astrophysical journal. Part 2, Letters
Year: 2023, Jahrgang: 943, Heft: 2, Pages: 1-6 |
| ISSN: | 2041-8213 |
| DOI: | 10.3847/2041-8213/acb157 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: https://doi.org/10.3847/2041-8213/acb157 Verlag, kostenfrei, Volltext: https://iopscience.iop.org/article/10.3847/2041-8213/acb157 
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| Verfasserangaben: | Peter Hoppe, Jan Leitner, Marco Pignatari, and Sachiko Amari |
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| 245 | 1 | 0 | |a New constraints for supernova models from presolar silicon carbide X grains with very high 26Al/27Al ratios |c Peter Hoppe, Jan Leitner, Marco Pignatari, and Sachiko Amari |
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| 246 | 3 | 3 | |a New constraints for supernova models from presolar silicon carbide X grains with very high 26 Al/27 Al ratios |
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| 520 | |a We report C, N, Mg-Al, Si, and S isotope data of six 1-3 μm-sized SiC grains of Type X from the Murchison CM2 chondrite, believed to have formed in the ejecta of core-collapse supernova (CCSN) explosions. Their C, N, and Si isotopic compositions are fully compatible with previously studied X grains. Magnesium is essentially monoisotopic 26Mg which gives clear evidence for the decay of radioactive 26Al. Inferred initial 26Al/27Al ratios are between 0.6 and 0.78 which is at the upper end of previously observed ratios of X grains. Contamination with terrestrial or solar system Al apparently is low or absent, which makes the X grains from this study particularly interesting and useful for a quantitative comparison of Al isotope data with predictions from supernova models. The consistently high 26Al/27Al ratios observed here may suggest that the lower 26Al/27Al ratios of many X grains from the literature are the result of significant Al contamination and in part also of an improper quantification of 26Al. The real dispersion of 26Al/27Al ratios in X grains needs to be explored by future studies. The high observed 26Al/27Al ratios in this work provide a crucial constraint for the production of 26Al in CCSN models. We explored different CCSN models, including both “classical” and H ingestion CCSN models. It is found that the classical models cannot account for the high 26Al/27Al ratios observed here; in contrast, H ingestion models are able to reproduce the 26Al/27Al ratios along with C, N, and Si isotopic ratios reasonably well. | ||
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| 700 | 1 | |a Amari, Sachiko |e VerfasserIn |4 aut | |
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