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Prevalence of SED turndown among classical Be stars: Are all Be stars close binaries?

11 Dec 2019 • Klement Robert • Carciofi A. C. • Rivinius T. • Ignace R. • Matthews L. D. • Torstensson K. • Gies D. • Vieira R. G. • Richardson N. D. • de Souza A. Domiciano • Bjorkman J. E. • Hallinan G. • Faes D. M. • Mota B. • Gullingsrud A. D. • de Breuck C. • Kervella P. • Curé M. • Gunawan D.

Rapid rotation is a fundamental characteristic of classical Be stars and a crucial property allowing for the formation of their circumstellar disks. Past evolution in a mass and angular momentum transferring binary system offers a plausible solution to how Be stars attained their fast rotation... (read more)

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Prevalence of SED turndown among classical Be stars: Are all Be stars close binaries?

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