Linked from

The 20 pages that link to R-process, each with the reason it gives.

• Neutron starRelated: Neutron-rich merger ejecta can produce heavy elements through this process.

• Core-collapse supernovaRelated: Some core-collapse environments may contribute to this process and disperse newly formed nuclei.

• Uranium-238Related: Uranium-238 is produced through neutron-rich events involving rapid neutron capture.

• Multi-messenger astronomyRelated: Spectra of merger afterglows can test whether neutron-star collisions produce these elements.

• GW170817Related: The merger’s ejecta supplied evidence that neutron-star collisions forge heavy elements.

• Margaret BurbidgeRelated: B2FH distinguished this pathway from slow capture as another source of heavy elements.

• Binary neutron starRelated: Neutron-rich merger ejecta can synthesize r-process nuclei, including lanthanides.

• KilonovaRelated: Kilonova ejecta provide conditions for this process to synthesize heavy nuclei.

• Population II starRelated: Element patterns in some Population II stars reveal ancient r-process enrichment events.

• Presolar grainRelated: Some grain signatures have been used to investigate heavy-element production histories.

• Isotopes of uraniumRelated: It is a principal astrophysical process that creates the heavy nuclei from which uranium descends.