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High-mass stars in Milky Way clusters

Published online by Cambridge University Press:  28 July 2017

Ignacio Negueruela
Ignacio Negueruela*
Affiliation:
Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal Escuela Politécnica Superior, Universidad de Alicante Carretera de San Vicente del Raspeig s/n, E03690, San Vicente del Raspeig, Alicante, Spain email: ignacio.negueruela@ua.es
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Abstract

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Young 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.

Keywords

open cluster and associations: generalstars: massiveformationevolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S329: The Lives and Death-Throes of Massive Stars , November 2016 , pp. 271 - 278
Copyright
Copyright © International Astronomical Union 2017 

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