We perform the first detailed three-dimensional simulation of low Mach num-ber convection preceding thermonuclear ignition in a mixed H/He X-ray burst. Our simulations include a moderate-sized, approximate network that captures hydrogen and helium burning up through rp-process breakout. We look in detail at the difference between two- and three-dimensional convective fields, including the details of the turbulent convection
Context. Degenerate ignition of helium in low-mass stars at the end of the red giant branch phase le...
The Low Mach Number Approximation (LMNA) is applied to 2D hydrodynamical modeling of Type I X-ray bu...
We have modelled a dual shell flash (DSF) in a low-metallicity 1.5M ⊙ AGB star using the 3-dimension...
Type I X-ray bursts are thermonuclear explosions on the surfaces of neutron stars that can be used t...
Type I X-ray Bursts (XRBs) are thermonuclear explosions of accreted mate-rial on the surfaces of a n...
Movies of 2D slices through the 3D simulations for a 25 Msol main-sequence star. The left panel sho...
Movies of 2D slices through the 3D simulations for a 25 Msol main-sequence star. The left panel sho...
Context. We study turbulent convection during the core helium flash close to its peak by comparing t...
Context. We study turbulent convection during the core helium flash close to its peak by comparing t...
The dynamics of helium shell convection driven by nuclear burning establish the conditions for runaw...
Context. A realistic parametrization of convection and convective boundary mixing in conventional st...
Context. A realistic parametrization of convection and convective boundary mixing in conventional st...
Thermonuclear flashes of hydrogen and helium accreted onto neutron stars produce the frequently obse...
The role of convection in the core helium flash is simulated by two-dimensional eddies interacting w...
Thermonuclear flashes of hydrogen and helium accreted onto neutron stars produce the frequently obse...
Context. Degenerate ignition of helium in low-mass stars at the end of the red giant branch phase le...
The Low Mach Number Approximation (LMNA) is applied to 2D hydrodynamical modeling of Type I X-ray bu...
We have modelled a dual shell flash (DSF) in a low-metallicity 1.5M ⊙ AGB star using the 3-dimension...
Type I X-ray bursts are thermonuclear explosions on the surfaces of neutron stars that can be used t...
Type I X-ray Bursts (XRBs) are thermonuclear explosions of accreted mate-rial on the surfaces of a n...
Movies of 2D slices through the 3D simulations for a 25 Msol main-sequence star. The left panel sho...
Movies of 2D slices through the 3D simulations for a 25 Msol main-sequence star. The left panel sho...
Context. We study turbulent convection during the core helium flash close to its peak by comparing t...
Context. We study turbulent convection during the core helium flash close to its peak by comparing t...
The dynamics of helium shell convection driven by nuclear burning establish the conditions for runaw...
Context. A realistic parametrization of convection and convective boundary mixing in conventional st...
Context. A realistic parametrization of convection and convective boundary mixing in conventional st...
Thermonuclear flashes of hydrogen and helium accreted onto neutron stars produce the frequently obse...
The role of convection in the core helium flash is simulated by two-dimensional eddies interacting w...
Thermonuclear flashes of hydrogen and helium accreted onto neutron stars produce the frequently obse...
Context. Degenerate ignition of helium in low-mass stars at the end of the red giant branch phase le...
The Low Mach Number Approximation (LMNA) is applied to 2D hydrodynamical modeling of Type I X-ray bu...
We have modelled a dual shell flash (DSF) in a low-metallicity 1.5M ⊙ AGB star using the 3-dimension...