Lorenzo's repositories
1-D-Supernova-shock-radius-evolution
A 1-D version of the ZEUS 2D CODE which solves hydrodynamic equations is applied to a SuperNova Remnant(SNR). The system is evolved for a time t =5x10^5 yrs and results are discussed below.
Metal-Diffusion-in-Galaxy-clusters
Simulation of metal diffusion in the ICM for the Perseus Cluster The aim of the project is to show the possible parameters for efficient metal distribution under reasonable diffusion timescales to reproduce observed abundance profile.
Radiative_cooling
Radiative cooling of an hydrogen-helium gas in collisional equilibrium of ionization.
galaxy_catalogue_analysis
Analysis of magnitude from a sample of galaxies from the SDSS3.
Hubble_constant
Determining the Value for the Hubble constant from a sample of Supernovae light curves given by the Canergie supernova project 2011.
lollocava00
Config files for my GitHub profile.