Burst timescales and luminosities as links between young pulsars and fast radio bursts
Fast radio bursts (FRBs) are extragalactic radio flashes of unknown physical origin. Their high luminosities and short durations require extreme energy densities, like those found in the vicinity of neutron stars and black holes. Studying the burst intensities and polarimetric properties on a wid...
Main Author: | Masui, Kiyoshi |
---|---|
Other Authors: | MIT Kavli Institute for Astrophysics and Space Research |
Format: | Article |
Language: | English |
Published: |
Springer Science and Business Media LLC
2022
|
Online Access: | https://hdl.handle.net/1721.1/142155 |
Similar Items
-
Modeling the Morphology of Fast Radio Bursts and Radio Pulsars with fitburst
by: E. Fonseca, et al.
Published: (2024-01-01) -
Fast Radio Burst Morphology in the First CHIME/FRB Catalog
by: Masui, Kiyoshi
Published: (2022) -
A repeating fast radio burst source in a globular cluster
by: Masui, Kiyoshi
Published: (2022) -
A second source of repeating fast radio bursts
by: The CHIME/FRB Collaboration, et al.
Published: (2022) -
CHIME/FRB Detection of the Original Repeating Fast Radio Burst Source FRB 121102
by: Masui, Kiyoshi
Published: (2022)