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Paper: Recent Development of the Current Be-Phase of Pleione
Volume: 361, Active OB-Stars: Laboratories For Stellar and Circumstellar Physics
Page: 440
Authors: Iliev, L.; Koubsky, P.; Kubat, J.; Kawka, A.
Abstract: We present results from the monitoring of spectral behavior of the Be/shell star Pleione in the period 2003–2005. The results from our observations again open the question for the timescale of quasi-periodic spectral changes of this star. Special emphasis is given on the variations of the Hα and Hβ emission lines.
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