FRB 121102: No supernova-like ejecta or magnetar power, hinting at a binary WD merger
astro-ph.HE, astro-ph.CO
Submitted: 2026-08-27
Updated: 2026-08-27
Terminology
Sources
- Milliarcsecond-scale spectrum of the persistent radio source associated with FRB 20190417A and constraints for FRB 20181030A
- The search for failed supernovae with the Large Binocular Telescope: confirmation of a disappearing star
- A flaring magnetar in FRB 121102?
- Constraints on the persistent radio source associated with FRB 20190520B using the European VLBI Network
- Quasi-steady emission from repeating fast radio bursts can be explained by magnetar wind nebulae
- A nebular origin for the persistent radio emission of fast radio bursts
- The direct localization of a fast radio burst and its host
- A comprehensive observational study of the FRB 121102 persistent radio source
- Common Envelope Evolution Leading to Supernovae with Dense Interaction
- The First CHIME/FRB Fast Radio Burst Catalog
- The CHIME Fast Radio Burst Project: System Overview
- Fast Radio Bursts: An Extragalactic Enigma
- Repeating behaviour of FRB 121102: periodicity, waiting times and energy distribution
- Indication for Decreasing Dispersion Measure in the Population of Repeating Fast Radio Bursts and Connection to Young Supernova Remnant Expansion
- The diverse outcomes of binary white dwarf mergers and connections to Galactic LISA sources
- Millisecond extragalactic radio bursts as magnetar flares
- Revisiting FRB 20121102A: milliarcsecond localisation and a decreasing dispersion measure
- Decadal evolution of a repeating fast radio burst source
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