Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S329(12), p. 271-278, 2016
DOI: 10.1017/s174392131700299x
Full text: Unavailable
AbstractYoung open clusters are our laboratories for studying high-mass star formation and evolution. Unfortunately, the information that they provide is difficult to interpret, and sometimes contradictory. In this contribution, I present a few examples of the uncertainties that we face when confronting observations with theoretical models and our own assumptions.