Abstract: Computes time and radial dependent magnetic fields for a sample of galaxies in the output of a semi-analytic model of galaxy formation. The magnetic field is obtained by numerically solving the galactic dynamo equations throughout history of each galaxy. Stokes parameters and Faraday rotation measure can also be computed along a random line-of-sight for each galaxy.
Credit: Rodrigues, Luiz F.S.; Chamandy, Luke
Preferred citation method: https://ui.adsabs.harvard.edu/abs/2019MNRAS.483.2424R