A Milliarcsecond Localization Associates FRB 20190417A with a Compact Persistent Radio Source and an Extreme Magnetoionic Environment
Artikel i vetenskaplig tidskrift, 2026

We report the milliarcsecond localization of a high (similar to 1379 pc cm(-3)) dispersion measure (DM) repeating fast radio burst (FRB), FRB 20190417A. Combining European VLBI Network detections of five repeat bursts, we confirm the FRB's host to be a low-metallicity, star-forming dwarf galaxy at z = 0.12817, similar to the hosts of FRB 20121102A, FRB 20190520B, and FRB 20240114A. We also confirm that it is associated with a previously reported persistent radio source (PRS), which is compact on milliarcsecond scales. Visibility-domain model fitting constrains the transverse physical size of the PRS to <23 pc and yields an integrated flux density of 190 +/- 40 mu Jy at 1.4 GHz. Though we do not find significant evidence for DM evolution, FRB 20190417A exhibits a time-variable rotation measure (RM) ranging between +3958 +/- 11 rad m(-2) and +5061 +/- 24 rad m(-2) over a 50-day period. We find no evidence for intervening galaxy clusters in the FRB's line of sight and place a conservative lower limit on the rest-frame host DM contribution of 1228 pc cm(-3) (90% confidence)-the largest known for any FRB so far. This system strengthens the emerging picture of a rare subclass of repeating FRBs with large and variable RMs, above-average host DMs, and luminous PRS counterparts in metal-poor dwarf galaxies. Our results suggest that these systems are the result of environmental selection, or a distinct engine for FRB emission.

Författare

Alexandra M. Moroianu

Universiteit Van Amsterdam

Shivani Bhandari

Commonwealth Scientific and Industrial Research Organisation (CSIRO)

Maria R. Drout

University of Toronto

Jason W. T. Hessels

Netherlands Institute for Radio Astronomy (ASTRON)

Universiteit Van Amsterdam

McGill University

Dante M. Hewitt

Universiteit Van Amsterdam

Franz Kirsten

Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium

Benito Marcote

Netherlands Institute for Radio Astronomy (ASTRON)

Joint Institute for VLBI in Europe (JIVE)

Ziggy Pleunis

Netherlands Institute for Radio Astronomy (ASTRON)

Universiteit Van Amsterdam

Mark P. Snelders

Netherlands Institute for Radio Astronomy (ASTRON)

Universiteit Van Amsterdam

Navin Sridhar

Stanford University

Uwe Bach

Max-Planck-Gesellschaft

Emmanuel K. Bempong-Manful

University of Bristol

University of Manchester

Vladislavs Bezrukovs

Ventspils University of Applied Sciences

Richard Blaauw

Netherlands Institute for Radio Astronomy (ASTRON)

Justin D. Bray

University of Manchester

Salvatore Buttaccio

Istituto nazionale di astrofisica (INAF)

Shami Chatterjee

Cornell University

Alessandro Corongiu

Istituto nazionale di astrofisica (INAF)

Roman Feiler

Uniwersytet Mikolaja Kopernika

B. M. Gaensler

University of Toronto

University of California

Marcin P. Gawronski

Uniwersytet Mikolaja Kopernika

Marcello Giroletti

Istituto nazionale di astrofisica (INAF)

Adaeze L. Ibik

University of Toronto

Ramesh Karuppusamy

Max-Planck-Gesellschaft

Mattias Lazda

University of Toronto

Calvin Leung

University of California

Michael Lindqvist

Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium

Kiyoshi W. Masui

Massachusetts Institute of Technology (MIT)

Daniele Michilli

Aix-Marseille Université

Kenzie Nimmo

Massachusetts Institute of Technology (MIT)

Omar S. Ould-Boukattine

Netherlands Institute for Radio Astronomy (ASTRON)

Universiteit Van Amsterdam

Ayush Pandhi

University of Toronto

Zsolt Paragi

Joint Institute for VLBI in Europe (JIVE)

Aaron B. Pearlman

McGill University

Weronika Puchalska

Uniwersytet Mikolaja Kopernika

Paul Scholz

University of Toronto

York University

Kaitlyn Shin

California Institute of Technology (Caltech)

Jurjen J. Sluman

Netherlands Institute for Radio Astronomy (ASTRON)

Matteo Trudu

Istituto nazionale di astrofisica (INAF)

David Williams-Baldwin

University of Manchester

Jun Yang

Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium

Astrophysical Journal Letters

2041-8205 (ISSN) 2041-8213 (eISSN)

Vol. 996 1 L16

Onsala rymdobservatorium infrastruktur

Vetenskapsrådet (VR) (2017-00648), 2018-01-01 -- 2021-12-31.

Ämneskategorier (SSIF 2025)

Astronomi, astrofysik och kosmologi

Meteorologi och atmosfärsvetenskap

DOI

10.3847/2041-8213/ae28c7

Mer information

Senast uppdaterat

2026-01-12