28 Canis Majoris - a short-period Be star.

Astronomy and Astrophysics – Astronomy

Scientific paper

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Be Stars:Spectra, Be Stars:Variations

Scientific paper

Are Be stars nothing but ß Cephei stars? This farreaching possibility is supported by new observations of the Be star 28 CMa, which shows spectral variations with aperiod of 1.36 days. Dr. Dietrich Baade of the Astronomical Institute of the University of Münster, FRG, recently obtained spectra of this star with the large coude spectrograph at the ESO 1.52 m te/escope. Here is his report about this important discovery.

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