Authors
                Dr.
            
                        Cyril Georgy
            
  Date and time
                                    19 Nov 2014 - 09:30 Europe/London
                            Address
                                    Aula
Talk language
                                    English
                            Serie number
                                    1
                            Description
                                    We will start by recalling the effects of rotation on stellar evolution and briefly explain its implementation in a stellar evolution code. We will present a set of various grids of massive stars models, and then show some recent results obtained by our new SYCLIST toolbox, which is able (among other things) to generate synthetic stellar clusters, including various physical ingredients, such as initial rotation and angle of view distributions, gravity and limb darkening, etc.