Lower-mass-gap Black Holes in Dense Star Clusters
The existence of compact stellar remnants in the mass range 2–5 M _⊙ has long been debated. This so-called lower-mass gap (LMG) was initially suggested by the lack of low-mass X-ray binary observations with accretors about 2–5 M _⊙ , but it has recently been called into question following newer obse...
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| Auteurs principaux: | , , , |
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| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
IOP Publishing
2024-01-01
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| Collection: | The Astrophysical Journal |
| Sujets: | |
| Accès en ligne: | https://doi.org/10.3847/1538-4357/ad76a0 |
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