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20192025
most citedThermal emission from bow shocks I: 2D Hydrodynamic Models of the Bubble Nebula

34 citations · 72 across the 6 of their papers we have counts for

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5 papers · 1 filter

astro-ph.GA2022

PION: Simulations of Wind-Blown Nebulae

Jonathan Mackey, Samuel Green, Maria Moutzouri +6

We present an overview of PION, an open-source software project for solving radiation-magnetohydrodynamics equations on a nested grid, aimed at modelling asymmetric nebulae around…

astro-ph.GA2022★ 13 cited

Thermal emission from bow shocks II: 3D magnetohydrodynamic models of Zeta Ophiuchi

S. Green, J. Mackey, P. Kavanagh +3

The nearby, massive, runaway star Zeta Ophiuchi has a large bow shock detected in optical and infrared, and, uniquely among runaway O stars, diffuse X-ray emission is detected from…

astro-ph.GA2021★ 16 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.GA2020★ 5 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.GA2019★ 34 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…