J
John M. Blondin
Researcher at North Carolina State University
Publications - 183
Citations - 10344
John M. Blondin is an academic researcher from North Carolina State University. The author has contributed to research in topics: Supernova & Supernova remnant. The author has an hindex of 56, co-authored 177 publications receiving 9739 citations. Previous affiliations of John M. Blondin include University of Chicago & University of Virginia.
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Stability of Standing Accretion Shocks, with an Eye toward Core-Collapse Supernovae
TL;DR: In this article, the stability of standing, spherical accretion shocks is examined in core-collapse supernovae, star formation, and accreting white dwarfs and neutron stars.
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Colliding Winds from Early-Type Stars in Binary Systems
TL;DR: In this article, a 2D hydrodynamics code was proposed to model the dynamics of the wind and shock structure formed by the collision in early-type binary systems, which self-consistently accounts for radiative cooling and represents a significant improvement over previous attempts to model these systems.
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Pulsar wind nebulae in evolved supernova remnants
TL;DR: In this paper, the authors have carried out one and two-dimensional, two-fluid simulations of the crushing and reexpansion phases of a pulsar wind nebula (PWN) and showed that these phases are subject to Rayleigh-Taylor instabilities that result in the mixing of thermal and nonthermal fluids, and asymmetries in the surrounding interstellar medium give rise to asymmetric in the position of the PWN relative to the pulsar and explosion site.
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Transition to the Radiative Phase in Supernova Remnants
TL;DR: In this paper, the evolution of a supernova remnant through the transition from an adiabatic Sedov-Taylor blast wave to a radiative pressure-driven snowplow phase is studied using one-and two-dimensional hydrodynamic simulations.
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Three-dimensional Core-collapse Supernova Simulated Using a 15 M⊙ Progenitor
Eric J. Lentz,Eric J. Lentz,Stephen W. Bruenn,W. Raphael Hix,W. Raphael Hix,Anthony Mezzacappa,Anthony Mezzacappa,O. E. Bronson Messer,O. E. Bronson Messer,O. E. Bronson Messer,Eirik Endeve,Eirik Endeve,John M. Blondin,J. Austin Harris,Pedro Marronetti,Konstantin N. Yakunin,Konstantin N. Yakunin +16 more
TL;DR: In this paper, the authors performed ab initio neutrino radiation hydrodynamics simulations in three and two spatial dimensions (3D and 2D) of core-collapse supernovae from the same 15 M⊙ progenitor through 440 ms after core bounce.