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Cited article:
W. Schmidt, J. C. Niemeyer, W. Hillebrandt
A&A, 450 1 (2006) 265-281
Published online: 2006-04-03
This article has been cited by the following article(s):
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Nucleosynthesis during a Thermonuclear Supernova Explosion
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Black hole formation in the early Universe
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3D deflagration simulations leaving bound remnants: a model for 2002cx-like Type Ia supernovae★
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Three‐Dimensional Simulations of the Deflagration Phase of the Gravitationally Confined Detonation Model of Type Ia Supernovae
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Rayleigh–Taylor unstable flames at higher Reynolds number
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EVOLUTION OF SHOCKS AND TURBULENCE IN MAJOR CLUSTER MERGERS
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A Three‐Dimensional Deflagration Model for Type Ia Supernovae Compared with Observations
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Type Ia supernova diversity: white dwarf central density as a secondary parameter in three-dimensional delayed detonation models
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Large-Scale Structure Formation: From the First Non-linear Objects to Massive Galaxy Clusters
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Hydrodynamical adaptive mesh refinement simulations of turbulent flows - I. Substructure in a wind
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On the applicability of the level set method beyond the
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Cosmological fluid mechanics with adaptively refined large eddy simulations
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THREE-DIMENSIONAL SIMULATIONS OF PURE DEFLAGRATION MODELS FOR THERMONUCLEAR SUPERNOVAE
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FOLLOWING THE COSMIC EVOLUTION OF PRISTINE GAS. I. IMPLICATIONS FOR MILKY WAY HALO STARS
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TURBULENCE IN A THREE-DIMENSIONAL DEFLAGRATION MODEL FOR TYPE Ia SUPERNOVAE. I. SCALING PROPERTIES
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Large-scale simulations of buoyancy-driven turbulent nuclear burning
D M Townsley, R A Bair, A Dubey, et al.
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TYPE Ia SUPERNOVA EXPLOSIONS FROM HYBRID CARBON–OXYGEN–NEON WHITE DWARF PROGENITORS
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Off‐Center Ignition in Type Ia Supernovae. I. Initial Evolution and Implications for Delayed Detonation
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ADAPTIVELY REFINED LARGE EDDY SIMULATIONS OF A GALAXY CLUSTER: TURBULENCE MODELING AND THE PHYSICS OF THE INTRACLUSTER MEDIUM
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The Astrophysical Journal 707 (1) 40 (2009)
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Combustion of a neutron star into a strange quark star: The neutrino signal
Giuseppe Pagliara, Matthias Herzog and Friedrich K. Röpke
Physical Review D 87 (10) (2013)
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THE DEFLAGRATION STAGE OF CHANDRASEKHAR MASS MODELS FOR TYPE Ia SUPERNOVAE. I. EARLY EVOLUTION
C. M. Malone, A. Nonaka, S. E. Woosley, et al.
The Astrophysical Journal 782 (1) 11 (2014)
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Turbulence in the ICM from mergers, cool-core sloshing, and jets: results from a new multi-scale filtering approach
F. Vazza, E. Roediger and M. Brüggen
Astronomy & Astrophysics 544 A103 (2012)
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CARBON DEFLAGRATION IN TYPE Ia SUPERNOVA. I. CENTRALLY IGNITED MODELS
H. Ma, S. E. Woosley, C. M. Malone, A. Almgren and J. Bell
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Adaptive mesh refinement simulations of a galaxy cluster merger – I. Resolving and modelling the turbulent flow in the cluster outskirts
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STUDY OF THE DETONATION PHASE IN THE GRAVITATIONALLY CONFINED DETONATION MODEL OF TYPE Ia SUPERNOVAE
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Modeling subgrid-scale force and divergence of heat flux of compressible isotropic turbulence by artificial neural network
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Modelling turbulent effects of stellar feedback in cosmological simulations
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High Performance Computing in Science and Engineering, Garching/Munich 2007
Luigi Iapichino, Jens C. Niemeyer, Julian Adamek, Surajit Paul and Mario Scuderi
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High Performance Computing in Science and Engineering, Garching/Munich 2007
Wolfram Schmidt, Andreas Maier, Markus Hupp, Christoph Federrath and Jens Niemeyer
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DOI: 10.1007/978-3-540-69182-2_7
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High Performance Computing in Science and Engineering, Garching/Munich 2009
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High Performance Computing in Science and Engineering, Garching/Munich 2009
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Interdisciplinary Aspects of Turbulence
F. Röpke and W. Schmidt
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Morphology of radio relics – I. What causes the substructure of synchrotron emission?
P Domínguez-Fernández, M Brüggen, F Vazza, et al.
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SN Ia Explosions from Hybrid Carbon–Oxygen–Neon White Dwarf Progenitors that Have Mixed during Cooling
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The Astrophysical Journal 887 (2) 188 (2019)
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THE FORMATION OF MASSIVE POPULATION III STARS IN THE PRESENCE OF TURBULENCE
M. A. Latif, D. R. G. Schleicher, W. Schmidt and J. Niemeyer
The Astrophysical Journal 772 (1) L3 (2013)
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Dynamic one-equation-based subgrid model for large-eddy simulation of stratified turbulent flows
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Grid-Based Hydrodynamics in Astrophysical Fluid Flows
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Amplification and generation of turbulence during self-gravitating collapse
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Radiative mixing layers: insights from turbulent combustion
Brent Tan, S Peng Oh and Max Gronke
Monthly Notices of the Royal Astronomical Society 502 (3) 3179 (2021)
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Cosmic-Ray Diffusion Suppression in Star-forming Regions Inhibits Clump Formation in Gas-rich Galaxies
Vadim A. Semenov, Andrey V. Kravtsov and Damiano Caprioli
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