Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S329(12), p. 271-278, 2016

DOI: 10.1017/s174392131700299x

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High-mass stars in Milky Way clusters

Journal article published in 2016 by Ignacio Negueruela ORCID
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

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Data provided by SHERPA/RoMEO

Abstract

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.

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