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Feedback from winds and supernovae in massive stellar clusters - I. Hydrodynamics

Monthly notices of the Royal Astronomical Society, 2013-05, Vol.431 (2), p.1337-1351

2013

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3D models of radiatively driven colliding winds in massive O+O star binaries – I. Hydrodynamics

Monthly notices of the Royal Astronomical Society, 2009-07, Vol.396 (3), p.1743-1763

Pittard, J. M.

2009

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The turbulent destruction of clouds – III. Three-dimensional adiabatic shock–cloud simulations

Monthly notices of the Royal Astronomical Society, 2016-04, Vol.457 (4), p.4470-4498

2016

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Thermal instability revisited

Monthly notices of the Royal Astronomical Society, 2020-03, Vol.492 (3), p.4484-4499

2020

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A comparison of shock–cloud and wind–cloud interactions: effect of increased cloud density contrast on cloud evolution

Monthly notices of the Royal Astronomical Society, 2018-05, Vol.476 (2), p.2209-2219

2018

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3D models of radiatively driven colliding winds in massive O + O star binaries – III. Thermal X-ray emission

Monthly notices of the Royal Astronomical Society, 2010-04, Vol.403 (4), p.1657-1683

2010

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3D models of radiatively driven colliding winds in massive O + O star binaries – II. Thermal radio to submillimetre emission

Monthly notices of the Royal Astronomical Society, 2010-04, Vol.403 (4), p.1633-1656

Pittard, J. M.

2010

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A Clumping-independent Diagnostic of Stellar Mass-Loss Rates: Rapid Clump Destruction in Adiabatic Colliding Winds

The Astrophysical journal, 2007-05, Vol.660 (2), p.L141-L144

Pittard, J. M

2007

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Magnetohydrodynamical simulation of the formation of clumps and filaments in quiescent diffuse medium by thermal instability

Monthly notices of the Royal Astronomical Society, 2016-06, Vol.459 (2), p.1803-1818

2016

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Numerical simulations of a shock-filament interaction

Monthly notices of the Royal Astronomical Society, 2016-05, Vol.458 (2), p.1139-1163

2016

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Momentum and energy injection by a wind-blown bubble into an inhomogeneous interstellar medium

Monthly notices of the Royal Astronomical Society, 2022-09, Vol.515 (2), p.1815-1829

Pittard, J M

2022

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Momentum and energy injection by a supernova remnant into an inhomogeneous medium

Monthly notices of the Royal Astronomical Society, 2019-09, Vol.488 (3), p.3376-3395

Pittard, J M

2019

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V444 Cygni X-ray and polarimetric variability: Radiative and Coriolis forces shape the wind collision region

Astronomy and astrophysics (Berlin), 2015-01, Vol.573, p.A43

2015

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Colliding stellar winds structure and X-ray emission

Monthly notices of the Royal Astronomical Society, 2018-07, Vol.477 (4), p.5640-5645

2018

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The turbulent destruction of clouds – II. Mach number dependence, mass-loss rates and tail formation

Monthly notices of the Royal Astronomical Society, 2010-06, Vol.405 (2), p.821-838

2010

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Numerical simulations of shocks encountering clumpy regions

Monthly notices of the Royal Astronomical Society, 2012-09, Vol.425 (3), p.2212-2227

2012

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A 3D dynamical model of the colliding winds in binary systems

Monthly notices of the Royal Astronomical Society, 2008-08, Vol.388 (3), p.1047-1061

2008

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Particle acceleration and non-thermal emission in colliding-wind binary systems

Monthly notices of the Royal Astronomical Society, 2021-07, Vol.504 (3), p.4204-4225

2021

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Feedback from winds and supernovae in massive stellar clusters – II. X-ray emission

Monthly notices of the Royal Astronomical Society, 2014-06, Vol.441 (2), p.964-982

2014

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How to inflate a wind-blown bubble

Monthly notices of the Royal Astronomical Society, 2021-12, Vol.508 (2), p.1768-1776

2021

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An exploration of dust grain growth within WCd systems using an advected scalar dust model

Monthly notices of the Royal Astronomical Society, 2022-10, Vol.516 (4), p.6132-6144

2022

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Radio emission models of colliding-wind binary systems. inclusion of IC cooling

Astronomy and astrophysics (Berlin), 2006-02, Vol.446 (3), p.1001-1019

2006

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Exploring dust growth in the episodic WCd system WR140

Monthly notices of the Royal Astronomical Society, 2022-11, Vol.517 (4), p.4705-4713

2022

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Colliding-wind binary systems: diffusive shock acceleration and non-thermal emission

Monthly notices of the Royal Astronomical Society, 2020-06, Vol.495 (2), p.2205-2221

2020

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How D-type H ii region expansion depends on numerical resolution

Monthly notices of the Royal Astronomical Society, 2022-02, Vol.510 (2), p.2797-2801

2022

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Feedback from winds and supernovae in massive stellar clusters - I. Hydrodynamics

3D models of radiatively driven colliding winds in massive O+O star binaries – I. Hydrodynamics

The turbulent destruction of clouds – III. Three-dimensional adiabatic shock–cloud simulations

Thermal instability revisited

A comparison of shock–cloud and wind–cloud interactions: effect of increased cloud density contrast on cloud evolution

3D models of radiatively driven colliding winds in massive O + O star binaries – III. Thermal X-ray emission

3D models of radiatively driven colliding winds in massive O + O star binaries – II. Thermal radio to submillimetre emission

A Clumping-independent Diagnostic of Stellar Mass-Loss Rates: Rapid Clump Destruction in Adiabatic Colliding Winds

Magnetohydrodynamical simulation of the formation of clumps and filaments in quiescent diffuse medium by thermal instability

Numerical simulations of a shock-filament interaction

Momentum and energy injection by a wind-blown bubble into an inhomogeneous interstellar medium

Momentum and energy injection by a supernova remnant into an inhomogeneous medium

V444 Cygni X-ray and polarimetric variability: Radiative and Coriolis forces shape the wind collision region

Colliding stellar winds structure and X-ray emission

The turbulent destruction of clouds – II. Mach number dependence, mass-loss rates and tail formation

Numerical simulations of shocks encountering clumpy regions

A 3D dynamical model of the colliding winds in binary systems

Particle acceleration and non-thermal emission in colliding-wind binary systems

Feedback from winds and supernovae in massive stellar clusters – II. X-ray emission

How to inflate a wind-blown bubble

An exploration of dust grain growth within WCd systems using an advected scalar dust model

Radio emission models of colliding-wind binary systems. inclusion of IC cooling

Exploring dust growth in the episodic WCd system WR140

Colliding-wind binary systems: diffusive shock acceleration and non-thermal emission

How D-type H ii region expansion depends on numerical resolution

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