Volume 344 - 14th European VLBI Network Symposium & Users Meeting (EVN2018) - Fast Transients, Neutron Stars & Pulsars Session
Localizations of Fast Radio Bursts on milliarcsecond scales
B. Marcote,* Z. Paragi
*corresponding author
Full text: pdf
Pre-published on: March 26, 2019
Published on: October 09, 2019
Abstract
Fast Radio Bursts (FRBs) are transient sources that emit a single radio pulse with a duration of only a few milliseconds. Since the discovery of the first FRB in 2007, tens of similar events have been detected. However, their physical origin remains unclear, and a number of scenarios even larger than the number of known FRBs has been proposed during these years. The detection of multiple bursts in FRB 121102 excluded all cataclysmic scenarios, at least for this particular FRB. The presence of these repeating bursts allowed us to perform a precise localization of the source with the Karl G. Jansky Very Large Array (VLA) and the European VLBI Network (EVN). Optical observations with Keck, Gemini and HST unveiled the host to be a low-metallicity star-forming dwarf galaxy located at a redshift of 0.193. The EVN results showed that the bursts are co-located (within a projected separation of $< 40$ pc) to a compact and persistent radio source with a size of $< 0.7$ pc and located within a star-forming region. This environment resembles the ones where superluminous supernovae or long-duration gamma-ray bursts are produced. Although the nature of this persistent source and the origin of the bursts remain unknown, the scenarios considering a neutron star/magnetar energizing a young superluminous supernova, or a system with a pulsar/magnetar in the vicinity of a massive black hole are the most plausible ones to date. More recent observations have shown that the bursts from FRB 121102 are almost 100% linearly polarized at an unexpectedly high and variable Faraday rotation measure, that has been observed to date only in vicinities of massive/supermassive black holes. The bursts are thus likely produced from a neutron star in such environment, although the system can still be explained by a young neutron star embedded in a highly magnetized pulsar wind nebula or supernova remnant. New FRB localizations would unveil if this source is representative of the whole population or a particular case. Upcoming interferometric searches are expected to report tens of these localizations in the coming years, dramatically boosting the field of FRBs.
DOI: https://doi.org/10.22323/1.344.0013
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