We present a multidimensional radiation magnetohydrodynamics (MHD) code based on the high-resolution shock capturing schemes (HRSC), the flux-limited diffusion (FLD) approximation, and the assumption of local thermodynamic equilibrium (LTE). The HRSC, employing a conservative algorithm that accurately ensures conservation of the total energy of MHD is implemented using a third-order Runge-Kutte scheme and the HLLD Riemann solver. In the FLD approximation, because the evolution equations of the radiation energy flux are neglected, this code is easily implemented, though the FLD approximation is less accurate when dealing with highly anisotropic radiation fields in an optically thin region. We carried out classical tests for the MHD and for t...
The development, testing, and application of a two dimensional radiation magnetohydrodynamics (RMHD)...
A numerical scheme is described for including radiation in multidimensional general relativistic con...
In this study we present a finite-volumen scheme for solving the equations of radiation magnetohydro...
We present a multidimensional numerical code to solve isothermal magnetohydrodynamic (IMHD) equation...
Aims. The transport of energy through radiation is very important in many astrophysical ph...
Aims. We describe a newly-developed magnetohydrodynamic (MHD) code with the capacity to simulate th...
International audienceContext. Radiation controls the dynamics and energetics of many astrophysical ...
In this, the third of a series of three papers, we conclude a detailed description of ZEUS-2D, a num...
Context. Radiative feedback plays a crucial role in the formation of massive stars. The implementa...
Context. Modeling the dynamics of most astrophysical structures requires an adequate description of ...
Aims. The transport of energy through radiation is very important in many astrophysical phenomena. I...
Context. Radiative feedback plays a crucial role in the formation of massive stars. The implementati...
Radiation feedback plays a crucial role in the process of star formation. In order to simulate the t...
Aims. The importance of radiation to the physical structure of protoplanetary disks cannot be unders...
We briefly overview our newly developed radiation transport module for MHD simulations and two actua...
The development, testing, and application of a two dimensional radiation magnetohydrodynamics (RMHD)...
A numerical scheme is described for including radiation in multidimensional general relativistic con...
In this study we present a finite-volumen scheme for solving the equations of radiation magnetohydro...
We present a multidimensional numerical code to solve isothermal magnetohydrodynamic (IMHD) equation...
Aims. The transport of energy through radiation is very important in many astrophysical ph...
Aims. We describe a newly-developed magnetohydrodynamic (MHD) code with the capacity to simulate th...
International audienceContext. Radiation controls the dynamics and energetics of many astrophysical ...
In this, the third of a series of three papers, we conclude a detailed description of ZEUS-2D, a num...
Context. Radiative feedback plays a crucial role in the formation of massive stars. The implementa...
Context. Modeling the dynamics of most astrophysical structures requires an adequate description of ...
Aims. The transport of energy through radiation is very important in many astrophysical phenomena. I...
Context. Radiative feedback plays a crucial role in the formation of massive stars. The implementati...
Radiation feedback plays a crucial role in the process of star formation. In order to simulate the t...
Aims. The importance of radiation to the physical structure of protoplanetary disks cannot be unders...
We briefly overview our newly developed radiation transport module for MHD simulations and two actua...
The development, testing, and application of a two dimensional radiation magnetohydrodynamics (RMHD)...
A numerical scheme is described for including radiation in multidimensional general relativistic con...
In this study we present a finite-volumen scheme for solving the equations of radiation magnetohydro...