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Miroslav Mocak
Miroslav Mocak
Software Enginner
Bestätigte E-Mail-Adresse bei ness.com - Startseite
Titel
Zitiert von
Zitiert von
Jahr
The core helium flash revisited-II. Two and three-dimensional hydrodynamic simulations
M Mocak, E Müller, A Weiss, K Kifonidis
Astronomy & Astrophysics 501 (2), 659-677, 2009
852009
The core helium flash revisited-I. One and two-dimensional hydrodynamic simulations
M Mocák, E Müller, A Weiss, K Kifonidis
Astronomy & Astrophysics 490 (1), 265-277, 2008
572008
The core helium flash revisited-III. From Population I to Population III stars
M Mocak, SW Campbell, E Mueller, K Kifonidis
Astronomy & Astrophysics 520, A114, 2010
492010
The core helium flash revisited-III. From Population I to Population III stars
M Mocak, SW Campbell, E Mueller, K Kifonidis
Astronomy & Astrophysics 520, A114, 2010
492010
Multidimensional hydrodynamic simulations of the hydrogen injection flash
M Mocak, L Siess, E Müller
Astronomy & Astrophysics 533, A53, 2011
312011
Turbulent mixing and nuclear burning in stellar interiors
M Mocák, C Meakin, SW Campbell, WD Arnett
Monthly Notices of the Royal Astronomical Society 481 (3), 2918-2932, 2018
272018
3D Simulations and MLT. I. Renzini’s critique
WD Arnett, C Meakin, R Hirschi, A Cristini, C Georgy, S Campbell, ...
The Astrophysical Journal 882 (1), 18, 2019
252019
Dynamics in a stellar convective layer and at its boundary: Comparison of five 3D hydrodynamics codes
R Andrassy, J Higl, H Mao, M Mocák, DG Vlaykov, WD Arnett, I Baraffe, ...
Astronomy & Astrophysics 659, A193, 2022
162022
A new stellar mixing process operating below shell convection zones following off-center ignition
M Mocak, CA Meakin, E Müller, L Siess
The Astrophysical Journal 743 (1), 55, 2011
142011
Compressible hydrodynamic mean-field equations in spherical geometry and their application to turbulent stellar convection data
M Mocák, C Meakin, M Viallet, D Arnett
arXiv preprint arXiv:1401.5176, 2014
42014
Hydrodynamic simulations of shell convection in stellar cores
M Mocák, E Müller, L Siess
Red Giants as Probes of the Structure and Evolution of the Milky Way, 87-93, 2011
22011
3D Simulations and MLT: II. Onsager's Ideal Turbulence
WD Arnett, R Hirschi, SW Campbell, M Mocák, C Georgy, C Meakin, ...
arXiv preprint arXiv:1810.04659, 2018
12018
Multidimensional hydrodynamic simulations of the core helium flash in low-mass stars
M Mocák
Technische Universität München, 2009
12009
3D hydrodynamics simulations of massive stars with the PROMPI code
F Rizzuti, R Hirschi, C Georgy, WD Arnett, C Meakin, M Mocák
Journal of Physics: Conference Series 2207 (1), 012048, 2022
2022
The Core Helium Flash: 3D Hydrodynamic Models
M Mocák, E Müller
High Performance Computing in Science and Engineering, Garching/Munich 2009 …, 2010
2010
Rayleigh-Taylor finger instability mixing in hydrodynamic shell convection models
M Mocak, E Mueller
arXiv preprint arXiv:1005.2295, 2010
2010
The Onset of Convection During the Core Helium Flash
M Mocák, E Müller
High Performance Computing in Science and Engineering, Garching/Munich 2007 …, 2009
2009
Hydrodynamic simulations of the core helium flash
M Mocák, E Müller, A Weiss, K Kifonidis
Proceedings of the International Astronomical Union 4 (S252), 215-221, 2008
2008
Multidimensional hydrodynamic simulations of the core helium ash
M Mocak, E Müller, A Weiss, K Kifonidis
TURBULENT CONVECTION IN STELLAR INTERIORS. IV. BALANCE EQUATIONS FOR TURBULENT TRANSPORT
M Mocak, CA Meakin, M Viallet, D Arnett
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