Cosmic ray feedback in galaxies and galaxy clusters: A pedagogical introduction and a topical review of the acceleration, transport, observables, and dynamical …

M Ruszkowski, C Pfrommer - The Astronomy and Astrophysics Review, 2023 - Springer
Understanding the physical mechanisms that control galaxy formation is a fundamental
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …

The discovery and scientific potential of fast radio bursts

M Bailes - Science, 2022 - science.org
Fast radio bursts (FRBs) are millisecond-time-scale bursts of coherent radio emission that
are luminous enough to be detectable at cosmological distances. In this Review, I describe …

A fast radio burst localized to a massive galaxy

V Ravi, M Catha, L D'addario, SG Djorgovski… - Nature, 2019 - nature.com
Intense, millisecond-duration bursts of radio waves (named fast radio bursts) have been
detected from beyond the Milky Way. Their dispersion measures—which are greater than …

Faraday depolarization and induced circular polarization by multipath propagation with application to FRBs

P Beniamini, P Kumar, R Narayan - Monthly Notices of the Royal …, 2022 - academic.oup.com
We describe how the observed polarization properties of an astronomical object are related
to its intrinsic polarization properties and the finite temporal and spectral resolutions of the …

A new measurement of the Hubble constant using fast radio bursts

S Hagstotz, R Reischke, R Lilow - Monthly Notices of the Royal …, 2022 - academic.oup.com
Fast radio bursts (FRBs) are very short and bright transients visible over extragalactic
distances. The radio pulse undergoes dispersion caused by free electrons, along the line of …

Magnetic fields on FIRE: Comparing B-fields in the multiphase ISM and CGM of simulated L* galaxies to observations

SB Ponnada, GV Panopoulou, IS Butsky… - Monthly Notices of …, 2022 - academic.oup.com
The physics of magnetic fields (B) and cosmic rays (CRs) have recently been included in
simulations of galaxy formation. However, significant uncertainties remain in how these …

On the fast radio burst and persistent radio source populations

CJ Law, L Connor, K Aggarwal - The Astrophysical Journal, 2022 - iopscience.iop.org
The first fast radio burst (FRB) to be precisely localized was associated with a luminous
persistent radio source (PRS). Recently, a second FRB/PRS association was discovered for …

Multiwavelength observations of fast radio bursts

L Nicastro, C Guidorzi, E Palazzi, L Zampieri, M Turatto… - Universe, 2021 - mdpi.com
The origin and phenomenology of the Fast Radio Burst (FRB) remains unknown despite
more than a decade of efforts. Though several models have been proposed to explain the …

Turbulent pressure support and hydrostatic mass bias in the intracluster medium

M Angelinelli, F Vazza, C Giocoli, S Ettori… - Monthly Notices of …, 2020 - academic.oup.com
The degree of turbulent pressure support by residual gas motions in galaxy clusters is not
well known. Mass modelling of combined X-ray and Sunyaev–Zel'dovich observations …

The cosmic baryon partition between the IGM and CGM in the SIMBA simulations

IS Khrykin, D Sorini, KG Lee… - Monthly Notices of the …, 2024 - academic.oup.com
We use the simba suite of cosmological hydrodynamical simulations to investigate the
importance of various stellar and active galactic nuclei (AGN) feedback mechanisms in …