Multiwavelength constraints on the origin of a nearby repeating fast radio burst source in a globular cluster
Artikel i vetenskaplig tidskrift, 2024

The precise origins of fast radio bursts (FRBs) remain unknown. Multiwavelength observations of nearby FRB sources can provide important insights into the enigmatic FRB phenomenon. Here we present results from a sensitive, broadband X-ray and radio observational campaign of FRB 20200120E, the closest known extragalactic repeating FRB source (located 3.63 Mpc away in an similar to 10-Gyr-old globular cluster). We place deep limits on the persistent and prompt X-ray emission from FRB 20200120E, which we use to constrain possible origins for the source. We compare our results with various classes of X-ray sources, transients and FRB models. We find that FRB 20200120E is unlikely to be associated with ultraluminous X-ray bursts, magnetar-like giant flares or an SGR 1935+2154-like intermediate flare. Although other types of bright magnetar-like intermediate flares and short X-ray bursts would have been detectable from FRB 20200120E during our observations, we cannot entirely rule them out as a class. We show that FRB 20200120E is unlikely to be powered by an ultraluminous X-ray source or a young extragalactic pulsar embedded in a Crab-like nebula. We also provide new constraints on the compatibility of FRB 20200120E with accretion-based FRB models involving X-ray binaries. These results highlight the power of multiwavelength observations of nearby FRBs for discriminating between FRB models.

Författare

Aaron B. Pearlman

California Institute of Technology (Caltech)

McGill University

Paul Scholz

University of Toronto

York University

Suryarao Bethapudi

Max-Planck-Gesellschaft

Jason W. T. Hessels

McGill University

Universiteit Van Amsterdam

Netherlands Inst Radio Astron

Victoria M. Kaspi

McGill University

Franz Kirsten

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

Kenzie Nimmo

Massachusetts Institute of Technology (MIT)

Laura G. Spitler

Max-Planck-Gesellschaft

Emmanuel Fonseca

West Virginia University

Bradley W. Meyers

University of British Columbia (UBC)

Curtin University

Ingrid H. Stairs

University of British Columbia (UBC)

Chia Min Tan

Curtin University

McGill University

Mohit Bhardwaj

Carnegie Mellon Univ, McWilliams Ctr Cosmol, Dept Phys

Shami Chatterjee

Cornell University

Amanda M. Cook

University of Toronto

Alice P. Curtin

McGill University

Fengqiu Adam Dong

University of British Columbia (UBC)

Tarraneh Eftekhari

Northwestern Univ, Ctr Interdisciplinary Explorat & Res Astrophys, Dept Phys & Astron

B. M. Gaensler

University of Toronto

University of California at Santa Cruz

Tolga Guver

Istanbul Universitesi

Jane Kaczmarek

CSIRO Space & Astron

University of British Columbia (UBC)

Calvin Leung

University of California at Berkeley

Kiyoshi W. Masui

Massachusetts Institute of Technology (MIT)

Daniele Michilli

Massachusetts Institute of Technology (MIT)

Thomas A. Prince

California Institute of Technology (Caltech)

Ketan R. Sand

McGill University

Kaitlyn Shin

Massachusetts Institute of Technology (MIT)

Kendrick M. Smith

Perimeter Institute for Theoretical Physics

Shriharsh P. Tendulkar

Tata Institute of Fundamental Research

National Centre for Radio Astrophysics India

MaRS Ctr

NATURE ASTRONOMY

2397-3366 (ISSN)

Vol. In Press

Ämneskategorier

Meteorologi och atmosfärforskning

Astronomi, astrofysik och kosmologi

DOI

10.1038/s41550-024-02386-6

Mer information

Senast uppdaterat

2024-12-20