Characterizing Compact-object Binaries in the Lower Mass Gap with Gravitational Waves
The source binary of the gravitational-wave (GW) event GW230529, detected at the beginning of the fourth LIGO-Virgo-KAGRA observing run, was inferred to consist of a neutron star (NS) and a compact object in the lower mass gap, a purported gap between the most massive NSs (∼3 M _⊙ ) and least massiv...
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| Autors principals: | , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
IOP Publishing
2026-01-01
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| Col·lecció: | The Astrophysical Journal |
| Matèries: | |
| Accés en línia: | https://doi.org/10.3847/1538-4357/ae3829 |
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