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High time-resolution (∆T~2 min) observations of the B2V star γ Ori on the 2-m telescope at the Terskol Peak Observatory are presented. Regular components of line profile variations with periods from ~57 min to ~130 min are recorded. The nature of these variations is discussed.
Astrophysics – Springer Journals
Published: Mar 1, 2023
Keywords: stars; spectra — line profiles— variability; individual; γ Ori
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