Context. Be stars are rapid rotators surrounded by a gaseous disk envelope whose origin is still under debate. This envelope is responsible for observed emission lines and large infrared excess. Aims. To progress in the understanding of the physical processes involved in the disk formation, we estimate the disk parameters for a sample of Be...
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January 2019 (v1)Journal articleUploaded on: December 4, 2022
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September 2015 (v1)Journal article
International audience
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2012 (v1)Journal article
International audience
Uploaded on: December 3, 2022 -
January 17, 2022 (v1)Journal article
Differential Interferometry allows to obtain the differential visibility and phase, in addition to the spectrum. The differential phase contains important information about the structure and motion of stellar photosphere such as stellar spots and non-radial pulsations, and particularly the rotation. Thus, this interferometric observable...
Uploaded on: December 3, 2022