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On the use of the Fourier transform to determine the projected rotational velocity of line-profile variable B stars

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Astronomy & Astrophysics 569 A118 (2014)
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Accurate stellar rotational velocities using the Fourier transform of the cross correlation maximum

C. G. Díaz, J. F. González, H. Levato and M. Grosso
Astronomy & Astrophysics 531 A143 (2011)
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An optical study of X-ray sources in the old open clusters NGC 752 and NGC 6940

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DOI: 10.1051/0004-6361:20010767
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