Colour evolution of stellar populations up to 100 Myr according to different models and ingredients. Fixed parameters are indicated at the top while variable ones at the bottom. a) Comparison between SSPs built with Padova tracks and SSPs from Maraston (2005) for different metallicities. b) SSPs with Padova tracks including nebular emission compared to those without nebular emission. c) Same as in b) for CSPs. d) CSP models built with a Kroupa IMF and variable upper stellar mass limit. e) CSP models built with different metallicities. f) CSP models built with different slopes for the IMF above 0.5 M⊙. Age (Myr) is indicated at selected evolutionary stages in panels b) and c).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.