Closed haleygomez closed 7 years ago
this branch adds in a new outflow function which instead of being xSFR at each time step, is dependent on the stellar mass of the system. The function is described in Feldmann et al 2015, and Hopkins et al 2012.
this branch adds in a new outflow function which instead of being xSFR at each time step, is dependent on the stellar mass of the system. The function is described in Feldmann et al 2015, and Hopkins et al 2012.