We use cosmological simulations in order to study the effects of supernova (SN) feedback on the formation of a Milky Way-type galaxy of virial mass ∼1012 h−1 M. We analyse a set of simulations run with the code described by Scannapieco et al., where we have tested our star formation and feedback prescription using isolated galaxy models. Here, we extend this work by simulating the formation of a galaxy in its proper cosmological framework, focusing on the ability of the model to form a disc-like structure in rotational support. We find that SN feedback plays a fundamental role in the evolution of the simulated galaxy, efficiently regulating the star-formation activity, pressurizing the gas and generating mass-loaded galactic winds. T...
In this thesis I examine supernova feedback in hydrodynamical simulations of galaxy disks. Understan...
We present a series of high-resolution cosmological simulations1 of galaxy formation to z = 0, spann...
We present a series of high-resolution cosmological simulations1 of galaxy formation to z = 0, spann...
We use cosmological simulations in order to study the effects of supernova (SN) feedback on the form...
We introduce the Making Galaxies In a Cosmological Context (MAGICC) programme of smoothed particle h...
We study the formation of disc galaxies in a fully cosmological framework using adaptive mesh refine...
We study the formation of disc galaxies in a fully cosmological framework using adaptive mesh refine...
Using hydrodynamic simulations of disc-galaxy major mergers, we investigate the star formation histo...
We present a Supernova (SN) feedback model that succeeds at describing the chemical and energetic ef...
We study the formation of disc galaxies in a fully cosmological framework using adaptive mesh refine...
Context. What exactly controls star formation in the Galaxy remains controversial. In particular, th...
International audienceTo better understand the impact of supernova (SN) explosions on the evolution ...
International audienceTo better understand the impact of supernova (SN) explosions on the evolution ...
We present a set of hydrodynamical/N-body controlled simulations of isolated gas-rich galaxies that ...
International audienceTo better understand the impact of supernova (SN) explosions on the evolution ...
In this thesis I examine supernova feedback in hydrodynamical simulations of galaxy disks. Understan...
We present a series of high-resolution cosmological simulations1 of galaxy formation to z = 0, spann...
We present a series of high-resolution cosmological simulations1 of galaxy formation to z = 0, spann...
We use cosmological simulations in order to study the effects of supernova (SN) feedback on the form...
We introduce the Making Galaxies In a Cosmological Context (MAGICC) programme of smoothed particle h...
We study the formation of disc galaxies in a fully cosmological framework using adaptive mesh refine...
We study the formation of disc galaxies in a fully cosmological framework using adaptive mesh refine...
Using hydrodynamic simulations of disc-galaxy major mergers, we investigate the star formation histo...
We present a Supernova (SN) feedback model that succeeds at describing the chemical and energetic ef...
We study the formation of disc galaxies in a fully cosmological framework using adaptive mesh refine...
Context. What exactly controls star formation in the Galaxy remains controversial. In particular, th...
International audienceTo better understand the impact of supernova (SN) explosions on the evolution ...
International audienceTo better understand the impact of supernova (SN) explosions on the evolution ...
We present a set of hydrodynamical/N-body controlled simulations of isolated gas-rich galaxies that ...
International audienceTo better understand the impact of supernova (SN) explosions on the evolution ...
In this thesis I examine supernova feedback in hydrodynamical simulations of galaxy disks. Understan...
We present a series of high-resolution cosmological simulations1 of galaxy formation to z = 0, spann...
We present a series of high-resolution cosmological simulations1 of galaxy formation to z = 0, spann...