Does Nature Allow the Formation of Ultra-compact Black Hole X-Ray Binaries via the Accretion-induced Collapse of Neutron Stars?
The formation path to ultracompact X-ray binaries (UCXBs) with black hole (BH) accretors is still unclear. In the classical formation scenario, it is difficult to eject the massive envelope of the progenitor star of the BH via the common envelope process. Given that some neutron stars (NSs) in binar...
Main Authors: | Hai-Liang Chen, Thomas M. Tauris, Xuefei Chen, Zhanwen Han |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/acd4b8 |
Similar Items
-
Post-merger Gravitational-wave Signal from Neutron-star Binaries: A New Look at an Old Problem
by: Konrad Topolski, et al.
Published: (2023-01-01) -
A Channel to Form Fast-spinning Black Hole–Neutron Star Binary Mergers as Multimessenger Sources. II. Accretion-induced Spin-up
by: Zhen-Han-Tao Wang, et al.
Published: (2024-01-01) -
Wide Binaries with White Dwarf or Neutron Star Companions Discovered from Gaia DR3 and LAMOST
by: Xinlin Zhao, et al.
Published: (2024-01-01) -
Thermal Effects in Binary Neutron Star Mergers
by: Jacob Fields, 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)