activity
20102022
most citedA very-high-energy component deep in the Gamma-ray Burst afterglow

274 citations · 982 across the 28 of their papers we have counts for

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Showing astro-ph.GAShow all

11 papers · 1 filter

astro-ph.GA20221 cited

Interaction between massive star winds and the interstellar medium

Jonathan Mackey

Massive stars drive strong winds that impact the surrounding interstellar medium, producing parsec-scale bubbles for isolated stars and superbubbles around young clusters. These bu…

astro-ph.GA202116 cited

PION: Simulating bow shocks and circumstellar nebulae

Jonathan Mackey, Samuel Green, Maria Moutzouri +4

Expanding nebulae are produced by mass loss from stars, especially during late stages of evolution. Multi-dimensional simulation of these nebulae requires high resolution near the…

astro-ph.GA2021

Magnetic fields and Star Formation around HII regions: The S235 complex

R. Devaraj, D. P. Clemens, L. K. Dewangan +3

Magnetic fields are ubiquitous and essential in star formation. In particular, their role in regulating formation of stars across diverse environments like HII regions needs to be…

astro-ph.GA20205 cited

Simulations of Magnetised Stellar-Wind Bubbles

Jonathan Mackey, Samuel Green, Maria Moutzouri

Initial results are presented from 3D MHD modelling of stellar-wind bubbles around O stars moving supersonically through the ISM. We describe algorithm updates that enable high-res…

astro-ph.GA201934 cited

Thermal emission from bow shocks I: 2D Hydrodynamic Models of the Bubble Nebula

Samuel Green, Jonathan Mackey, Thomas J. Haworth +2

The Bubble Nebula (or NGC 7635) is a parsec-scale seemingly spherical wind-blown bubble around the relatively unevolved O star BD+602522. The small dynamical age of the neb…

astro-ph.GA2018

The classical D-type expansion of spherical H II regions

Robin J. R. Williams, Thomas G. Bisbas, Thomas J. Haworth +1

Recent numerical and analytic work has highlighted some shortcomings in our understanding of the dynamics of H II region expansion, especially at late times, when the H II region a…