Mass Transfer in Eccentric Black Hole–Neutron Star Mergers
Black hole–neutron star binaries are of interest in many ways: they are intrinsically transient, radiate gravitational waves detectable by LIGO, and may produce γ -ray bursts. Although it has long been assumed that their late-stage orbital evolution is driven entirely by gravitational wave emission,...
Guardat en:
| Autors principals: | , , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
IOP Publishing
2025-01-01
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| Col·lecció: | The Astrophysical Journal |
| Matèries: | |
| Accés en línia: | https://doi.org/10.3847/1538-4357/ad9b87 |
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