Black Hole Ultracompact X-Ray Binaries as Galactic Low-frequency Gravitational Wave Sources: The He Star Channel
Black hole (BH) ultracompact X-ray binaries (UCXBs) are potential Galactic low-frequency gravitational wave (GW) sources. As an alternative channel, BH UCXBs can evolve from BH+He star binaries. In this work, we perform a detailed stellar evolution model for the formation and evolution of BH UCXBs e...
Main Authors: | Ke Qin, Kun Xu, Dong-Dong Liu, Long Jiang, Bo Wang, Wen-Cong Chen |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2024-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/ad12d3 |
Similar Items
-
Black Hole Ultracompact X-Ray Binaries: Galactic Low-frequency Gravitational Wave Sources
by: Ke Qin, et al.
Published: (2023-01-01) -
Simulations of the Progenitors of Black Hole–Neutron Star Gravitational Wave Sources
by: Long Jiang, et al.
Published: (2023-01-01) -
Search for a Black Hole Binary in Gaia DR3 Astrometric Binary Stars with Spectroscopic Data
by: Ataru Tanikawa, et al.
Published: (2023-01-01) -
The Missing Link between Black Holes in High-mass X-Ray Binaries and Gravitational-wave Sources: Observational Selection Effects
by: Camille Liotine, et al.
Published: (2023-01-01) -
Compact Binary Coalescences: Astrophysical Processes and Lessons Learned
by: Mario Spera, et al.
Published: (2022-06-01)