Outcomes of stars depending on their stellar initial mass for NGC 288 and NGC 6366 using the CCSN model W18 of Sukhbold et al. (2016). Black shows mass ranges of failed CCSNe, red shows stars that explode as CCSNe and of which the iron is used in the formation of further stars and grey shows stars that explode as CCSNe after SF stopped. The time after which SF ends is marked by an arrow and written above the last star to explode.