A

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ARCOS , C

Last name: ARCOS

First name: C

January 2019 (v1)

Journal article

Metadata-only

Spectro-interferometric observations of a sample of Be stars Setting limits to the geometry and kinematics of stable Be disks

Cochetti, Y Arcos, C Kanaan, S.

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...

Uploaded on: December 4, 2022