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2011 (v1)Journal articleUploaded on: December 4, 2022
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2008 (v1)Journal article
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2015 (v1)Journal article
Stellar rotation is a key in our understanding of both mass-loss and evolution of intermediate and massive stars. It can lead to anisotropic mass-loss in the form of radiative wind or an excretion disk. We used the VEGA visible beam combiner installed on the CHARA array that reaches a sub milliarcsecond resolution. We derived, for the first...
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2012 (v1)Journal article
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2006 (v1)Conference paper
Advances in Stellar Interferometry, SPIE 6268, (2006)
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2012 (v1)Journal article
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2011 (v1)Journal article
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2011 (v1)Journal article
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2011 (v1)Journal article
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2011 (v1)Journal article
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2011 (v1)Journal article
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Uploaded on: December 3, 2022 -
2011 (v1)Journal article
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Uploaded on: December 3, 2022