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astro-ph.SR2022★ 3 cited
Angular Momentum Loss Rates in Be Stars Determined by the Viscous Decretion Disc Model
M. R. Ghoreyshi, C. E. Jones, A. Granada
Circumstellar discs around Be stars are formed by the material ejected by the central star. This process removes excess angular momentum from the star as viscosity facilitates the…
astro-ph.SR2022★ 3 cited
Simultaneous J-, H-, K- and L-band spectroscopic observations of galactic Be stars. I. IR atlas
Y. R. Cochetti, M. L. Arias, L. S. Cidale +2
It is already accepted that Be stars are surrounded by circumstellar envelopes, which are mostly compatible with a disc geometry in Keplerian rotation. We aim to obtain a more comp…