The Common Envelope Jet Supernova (CEJSN) r-process Scenario
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab1d5d/pdf
Reference81 articles.
1. Neutron star mergers versus core-collapse supernovae as dominant r-process sites in the early Galaxy
2. Black Hole Formation via Hypercritical Accretion during Common‐Envelope Evolution
3. Nuclear Composition of Gamma‐Ray Burst Fireballs
4. Retainment of r-process material in dwarf galaxies
5. r-PROCESS PRODUCTION SITES AS INFERRED FROM Eu ABUNDANCES IN DWARF GALAXIES
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2. Discovery of an Extremely r-process-enhanced Thin-disk Star with [Eu/H] = +0.78;The Astrophysical Journal Letters;2024-07-24
3. Chemical Diversity on Small Scales: Abundance Analysis of the Tucana V Ultrafaint Dwarf Galaxy;The Astrophysical Journal;2024-06-01
4. SPLUS J142445.34–254247.1: An r-process–enhanced, Actinide-boost, Extremely Metal-poor Star Observed with GHOST;The Astrophysical Journal;2023-12-01
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