Mass-gap Black Holes in Coalescing Neutron Star–Black Hole Binaries

Mass-gap Black Holes in Coalescing Neutron Star–Black Hole Binaries

The existence of a mass gap of 3–5 M _⊙ between the heaviest neutron stars (NSs) and the lightest black holes (BHs), inferred from the BH mass distribution in low-mass X-ray binaries (LMXBs), has been suggested for decades. The gravitational-wave (GW) source GW230529 is most likely a neutron star–bl...

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Bibliographic Details
Main Authors: Zepei Xing, Vicky Kalogera, Tassos Fragos, Jeff J. Andrews, Simone S. Bavera, Max Briel, Seth Gossage, Konstantinos Kovlakas, Matthias U. Kruckow, Kyle Akira Rocha, Meng Sun, Philipp M. Srivastava, Emmanouil Zapartas
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Gravitational waves
Neutron stars
Black holes
Online Access:https://doi.org/10.3847/1538-4357/adec6d
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https://doi.org/10.3847/1538-4357/adec6d

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