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On correlation of Hα, iron and oxygen line strengths in some B, Be and shell stars

S. M. Saad, J. Kubát, M. I. Nouh and M. A. Hamdy
Astrophysics and Space Science 325 (1) 7 (2010)
DOI: 10.1007/s10509-009-0165-9
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Evidence for Companion-induced Secular Changes in the Turbulent Disk of a Be Star in the Large Magellanic Cloud MACHO Database

Mitchell F. Struble, Anthony Galatola, Lorenzo Faccioli, Charles Alcock and Kelle Cruz
The Astronomical Journal 131 (4) 2196 (2006)
DOI: 10.1086/500806
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