Spin Evolution and Mass Distribution of Galactic Binary Neutron Stars
Binary neutron stars (BNSs) detected in the Milky Way have total masses distributing narrowly around ∼2.6–2.7 M _⊙ , while the BNS merger GW190425 detected via a gravitational wave has a significantly larger mass (∼3.4 M _⊙ ). This difference is not well understood, yet. In this paper, we investigat...
Saved in:
| Main Authors: | Qingbo Chu, Youjun Lu, Shenghua Yu |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ad90e2 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Modeling High Mass X-Ray Binaries to Double Neutron Stars through Common Envelope Evolution
by: Yu-Dong Nie, et al.
Published: (2025-01-01) -
Long-term Evolution of Sco X-1: Implications for the Current Spin Frequency and Ellipticity of the Neutron Star
by: Abhijnan Kar, et al.
Published: (2025-01-01) -
A Multimessenger Mass Determination Method for LISA Neutron Star–White Dwarf Binaries
by: Kaye Jiale Li, et al.
Published: (2025-01-01) -
X-Ray Polarization Study of the Neutron Star Low-mass X-Ray Binary GX 349+2
by: Unnati Kashyap, et al.
Published: (2025-01-01) -
X-Ray and Radio Polarimetry of the Neutron Star Low-mass X-Ray Binary 4U 1728–34
by: Unnati Kashyap, et al.
Published: (2025-01-01)