Document Type

Article

Publication Date

3-31-2022

Publication Title

The Astrophysical Journal Letters

First page number:

1

Last page number:

9

Abstract

Some repeating fast radio burst (FRB) sources exhibit complex polarization behaviors, including frequencydependent depolarization, variation of rotation measure (RM), and oscillating spectral structures of polarized components. Very recently, Feng et al. reported that active repeaters exhibit conspicuous frequency-dependent depolarization and a strong correlation between RM scatter (σRM) and the temporal scattering time (τs), s s 1.0 0.2, both of which can be well described by multipath propagation through a magnetized inhomogeneous plasma screen. This observation strongly suggests that the temporal scattering and RM scatter originate from the same region. Besides, a particular finding of note in Feng et al. is that the FRBs with compact persistent radio sources (PRSs) tend to have extreme σRM. In this work, we focus on some theoretical predictions of the relations among temporal scattering, depolarization by RM scatter, and PRSs contributed by the magnetized plasma environment close to a repeating FRB source. The behaviors of the RM scatter imply that the magnetized plasma environment is consistent with a supernova remnant or pulsar wind nebula, and the predicted σRM–τs relation is s RM µ ts 0.54 0.83 ( ) fordifferent astrophysical scenarios. We further make a general discussion of PRSs that does not depend on specific astrophysical scenarios. We show that the specific luminosity of a PRS should have a positive correlation with the RM contributed by the plasma screen. This is consistent with the observations of FRB 121102 and FRB 190520B.

Keywords

Systematics; taxonomy; genomics; ICNP; metagenomics; single-cell genomics; SeqCode; nomenclatural type; type

Disciplines

Astrophysics and Astronomy

File Format

pdf

File Size

481 KB

Language

English

Rights

IN COPYRIGHT. For more information about this rights statement, please visit http://rightsstatements.org/vocab/InC/1.0/

Creative Commons License

Creative Commons Attribution 4.0 International License
This work is licensed under a Creative Commons Attribution 4.0 International License.

Download

UNLV article access

Search your library

Share

COinS