Radioactive Gamma-Ray Lines from Long-lived Neutron Star Merger Remnants
The observation of a kilonova AT2017gfo associated with the gravitational wave event GW170817 provides the first strong evidence that neutron star mergers are dominant contributors to the production of heavy r -process elements. Radioactive gamma-ray lines emitted from neutron star merger remnants p...
Sábháilte in:
| Príomhchruthaitheoirí: | , , |
|---|---|
| Formáid: | Artigo |
| Teanga: | Inglês |
| Foilsithe / Cruthaithe: |
IOP Publishing
2024-01-01
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| Sraith: | The Astrophysical Journal |
| Ábhair: | |
| Rochtain ar líne: | https://doi.org/10.3847/1538-4357/ad65ec |
| Clibeanna: |
Níl clibeanna ann, Bí ar an gcéad duine le clib a chur leis an taifead seo!
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