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Title resolution pending

Bartos, I · 2019 · DOI 10.3847/2041-8213/ab3215

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fields

astro-ph.HE 1

years

2026 1

verdicts

UNVERDICTED 1

representative citing papers

The early r-process nucleosynthesis scenarios

astro-ph.HE · 2026-01-21 · unverdicted · novelty 3.0

Magnetorotational r-process best explains lighter elements and CEJSN explains the third peak based on scatter and iron correlations in early metal-poor stars.

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  • The early r-process nucleosynthesis scenarios astro-ph.HE · 2026-01-21 · unverdicted · none · ref 5

    Magnetorotational r-process best explains lighter elements and CEJSN explains the third peak based on scatter and iron correlations in early metal-poor stars.