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An interferometric journey around massive stars

Published online by Cambridge University Press:  23 January 2015

Anthony Meilland  and
Philippe Stee
Anthony Meilland
Affiliation:
Laboratoire Lagrange UMR7293 OCA - CNRS - UNS - Bd de l'Observatoire, Nice, France email: ame@oca.eu
Philippe Stee
Affiliation:
Laboratoire Lagrange UMR7293 OCA - CNRS - UNS - Bd de l'Observatoire, Nice, France email: ame@oca.eu
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Abstract

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Since the construction in the late nineties of modern facilities such as the VLTI or CHARA, interferometry became a key technique to probe massive stars and their often-complex circumstellar environments. Over the last decade, the development of a new generation of beam combiners for these facilities enabled major breakthroughs in the understanding of the formation and evolution of massive stars. In this short review, we will present few of these advances concerning young stellar objects, binarity, mass loss, and stellar surfaces.

Keywords

techniques: interferometricstars: binaries (including multiple): closestars: circumstellar matterstars: early-typestars: emission-lineBestars: mass lossstars: imaging
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Issue S307: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry , June 2014 , pp. 241 - 251
Copyright
Copyright © International Astronomical Union 2015 

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