Recent Development of the Current Be-Phase of Pleione

Details Recent Development of the Current Be-Phase of Pleione Recent Development of the Current Be-Phase of Pleione

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..361..440i&link_type=abstract

Active OB-Stars: Laboratories for Stellar and Circumstellar Physics, ASP Conference Series, Vol. 361, Proceedings of the confere

Physics

1

Scientific paper

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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