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Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2013, Volume 431, Issue 2, pp. 1337 - 1351
We use 3D hydrodynamical models to investigate the effects of massive star feedback from winds and supernovae on inhomogeneous molecular material left over... 
Supernovae: general | Hydrodynamics | ISM: general | RADIATION-PRESSURE | STAR-CLUSTERS | IONIZING FEEDBACK | hydrodynamics | INTERSTELLAR-MEDIUM | supernovae: general | TURBULENT DESTRUCTION | GIANT MOLECULAR CLOUDS | BLOWN BUBBLES | ASTRONOMY & ASTROPHYSICS | SELF-SIMILAR EVOLUTION | NUMERICAL SIMULATIONS | HII-REGIONS
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 07/2018, Volume 477, Issue 4, pp. 5640 - 5645
We investigate the structure and X-ray emission from the colliding stellar winds in massive star binaries. We find that the opening angle of the contact... 
Shock waves | X-rays: stars | Stars: mass-loss | Stars: winds | Stars: early-type | Binaries: general | Outflows | WR 140 | ETA-CARINAE | BINARY-SYSTEMS | COLLISION | stars: winds, outflows | SHOCKS | MINIMUM | stars: early-type | EARLY-TYPE STARS | ASTRONOMY & ASTROPHYSICS | stars: mass-loss | XMM-NEWTON OBSERVATIONS | binaries: general | RADIATIVE BRAKING | MASS-LOSS | shock waves
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2009, Volume 396, Issue 3, pp. 1743 - 1763
The dynamics of the wind-wind collision in massive stellar binaries are investigated using 3D hydrodynamical models which incorporate gravity, the driving of... 
hydrodynamics | binaries: general | stars: mass‐loss | stars: winds, outflows | shock waves | stars: early‐type | Shock waves | Hydrodynamics | Stars: winds, outflows | Stars: mass-loss | Stars: early-type | Binaries: general | Fluid dynamics | Analysis | Models | Astrophysics | Double stars | Physics - Solar and Stellar Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2016, Volume 457, Issue 4, pp. 4470 - 4498
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2017, Volume 470, Issue 2, pp. 2427 - 2438
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 458, Issue 2, pp. 1139 - 1163
We present 3D hydrodynamic adiabatic simulations of a shock interacting with a dense, elongated cloud. We compare how the nature of the interaction changes... 
Shock waves | Hydrodynamics | Turbulence | ISM: Kinematics and dynamics | ISM: Clouds | ISM: Supernova remnants | Physics - Astrophysics of Galaxies
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2001, Volume 383, Issue 2, pp. 636 - 647
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 05/2018, Volume 476, Issue 2, pp. 2209 - 2219
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2016, Volume 461, Issue 1, pp. 578 - 605
We present 3D magnetohydrodynamic numerical simulations of the adiabatic interaction of a shock with a dense, filamentary cloud. We investigate the effects of... 
MHD | Shockwaves | ISM: clouds | ISM: kinematics and dynamics | ISM: magnetic fields | HYDRODYNAMIC INTERACTION | THERMAL CONDUCTION | STAR-FORMATION | SUPERNOVA REMNANT | INTERSTELLAR CLOUDS | TURBULENT DESTRUCTION | GALAXY | GAS CLOUDS | ASTRONOMY & ASTROPHYSICS | NUMERICAL SIMULATIONS | shockwaves | Physics - Astrophysics of Galaxies
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2013, Volume 435, Issue 4, pp. 3600 - 3613
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2019, Volume 485, Issue 4, pp. 4686 - 4702
This paper describes 3D simulations of the formation of collapsing cold clumps via thermal instability inside a larger cloud complex. The initial condition was... 
Instabilities | ISM: Structure | ISM: Clouds | methods: Numerical | ISM: Molecules | stars: Formation | STAR-FORMATION | methods: numerical | SUPERNOVAE | instabilities | ISM: structure | stars: formation | ORIGIN | EVOLUTION | CLUSTERS | ISM: molecules | ASTRONOMY & ASTROPHYSICS | ISM: clouds | TURBULENCE | FLOWS | MECHANICAL STELLAR FEEDBACK | INTERSTELLAR ATOMIC-HYDROGEN
Journal Article
Monthly Notices of the Royal Astronomical Society: Letters, ISSN 1745-3925, 02/2011, Volume 411, Issue 1, pp. L41 - L45
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2017, Volume 470, Issue 2, pp. 2283 - 2313
We have used the AMR hydrodynamic code, MG, to perform 3D hydrodynamic simulations with self-gravity of stellar feedback in a spherical clumpy molecular cloud... 
ISM: supernova remnants | Stars: mass-loss | Stars: winds | Stars: massive | Hydrodynamics | ISM: clouds | Outflows | MASSIVE STARS | WINDS | hydrodynamics | INTERSTELLAR-MEDIUM | stars: winds, outflows | O-STARS | ISM:clouds | ENERGY-BALANCE | EVOLUTION | CLUSTERS | ASTRONOMY & ASTROPHYSICS | stars: mass-loss | stars: massive | SUPERNOVA-DRIVEN ISM | M-CIRCLE-DOT | Physics - Astrophysics of Galaxies
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2009, Volume 394, Issue 4, pp. 1758 - 1774
The X-ray emission from the supermassive star η Car is simulated using a 3D model of the wind-wind collision. In the model the intrinsic X-ray emission is... 
X‐rays: stars | binaries: close | hydrodynamics | stars: individual: η Carinae | stars: winds, outflows | stars: early‐type | ηCarinae-Stars | Winds | Hydrodynamics-Stars | Outflows-X-rays | Early-type-binaries | Individual | Stars | close-Stars
Journal Article