Massive stars at low metallicity - Evolution and surface abundances of O dwarfs in the SMC
Massive stars at low metallicity - Evolution and surface abundances of O dwarfs in the SMC
Aims. We aim to study the properties of massive stars at low metallicity, with an emphasis on their evolution, rotation, and surface abundances. We focus on O-type dwarfs in the Small Magellanic Cloud. These stars are expected to have weak winds that do not remove significant amounts of their initial …