Reconciling the Waiting Time Peaks Variations of Repeating FRBs with an Eccentric Neutron Star–White Dwarf Binary
Fast radio bursts (FRBs) are luminous radio transients with millisecond duration. For some active repeaters, such as FRBs 20121102A and 20201124A, more than a thousand bursts have been detected by the Five-hundred-meter Aperture Spherical radio Telescope (FAST). The waiting time (WT) distributions o...
Saved in:
| Main Author: | Hao-Yan Chen |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
MDPI AG
2025-04-01
|
| Series: | Universe |
| Subjects: | |
| Online Access: | https://www.mdpi.com/2218-1997/11/5/133 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
A Multimessenger Mass Determination Method for LISA Neutron Star–White Dwarf Binaries
by: Kaye Jiale Li, et al.
Published: (2025-01-01) -
A Massive White Dwarf or Low-mass Neutron Star Discovered by LAMOST
by: Xinlin Zhao, et al.
Published: (2024-01-01) -
A Unified Model of Kilonovae and Gamma-Ray Bursts in Binary Mergers Establishes Neutron Stars as the Central Engines of Short GRBs
by: Ore Gottlieb, et al.
Published: (2025-01-01) -
A New Brown Dwarf Orbiting an M Star and an Investigation of the Eccentricity Distribution of Transiting Long-period Brown Dwarfs
by: Tianjun Gan, et al.
Published: (2025-01-01) -
Spin Evolution and Mass Distribution of Galactic Binary Neutron Stars
by: Qingbo Chu, et al.
Published: (2025-01-01)