Radiation driven implosion and triggered star formation

Radiation driven winds with rotation: The oblate finite disc correction factor

Radiation Hydrodynamics in Solar Flares

Radiation hydrodynamics of core-collapse supernovae: the "key" asset for a self-consistent modelling of these events

Radiation Hydrodynamics of Line-Driven Winds

Radiation hydrodynamics of triggered star formation: the effect of the diffuse radiation field

Radiation Magnetohydrodynamics Simulation of Proto-Stellar Collapse: Two-Component Molecular Outflow

Radiation pressure and pulsation effects on the Roche lobe

Radiation pressure feedback in the formation of massive stars

Radiation thermo-chemical models of protoplanetary disks II. Line diagnostics

Radiation Transfer of Models of Massive Star Formation. I. Dependence on Basic Core Properties

Radiation-driven Implosion in the Cepheus B Molecular Cloud

Radiation-driven winds of hot luminous stars XVII. Parameters of selected central stars of PN from consistent optical and UV spectral analysis and the universality of the mass-luminosity relation

Radiation-driven winds of hot luminous stars. XVI. Expanding atmospheres of massive and very massive stars and the evolution of dense stellar clusters

Radiation-Hydrodynamic Models of the evolving Circumstellar Medium around Massive Stars

Radiation-Hydrodynamic Models of X-Ray & EUV Photoevaporating Protoplanetary Discs

Radiation-Hydrodynamic Simulations of Massive Star Formation with Protostellar Outflows

Radiation-Hydrodynamic Simulations of Protostellar Outflows: Synthetic Observations and Data Comparisons

Radiation-Hydrodynamic Simulations of the Formation of Orion-Like Star Clusters II. The Initial Mass Function from Winds, Turbulence, and Radiation

Radiation-hydrodynamical modelling of Core-Collapse Supernovae: light curves and the evolution of photospheric velocity and temperature