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Cited article:

Prevalence of SED Turndown among Classical Be Stars: Are All Be Stars Close Binaries?

Robert Klement, A. C. Carciofi, T. Rivinius, R. Ignace, L. D. Matthews, K. Torstensson, D. Gies, R. G. Vieira, N. D. Richardson, A. Domiciano de Souza, J. E. Bjorkman, G. Hallinan, D. M. Faes, B. Mota, A. D. Gullingsrud, C. de Breuck, P. Kervella, M. Curé and D. Gunawan
The Astrophysical Journal 885 (2) 147 (2019)
https://doi.org/10.3847/1538-4357/ab48e7

FAR-ULTRAVIOLET DETECTION OF THE SUSPECTED SUBDWARF COMPANION TO THE Be STAR 59 CYGNI

Geraldine J. Peters, Tiffany D. Pewett, Douglas R. Gies, Yamina N. Touhami and Erika D. Grundstrom
The Astrophysical Journal 765 (1) 2 (2013)
https://doi.org/10.1088/0004-637X/765/1/2