HD 45314 and HD 60848 are poorly studied Oe-type stars. Spectroscopic monitoring over 5 years reveals strong variations in the strength of the emission lines and for HD 45314 in the V/R ratio of the double-peaked emissions. Part of these long-term variations could be recurrent

De Becker, Michaël

Marique, P. X.

Nazé, Yaël

Rauw, Grégor

Sana, Hugues

Vreux, Jean-Marie

peer reviewedHD 45314 and HD 60848 are poorly studied Oe-type stars. Spectroscopic monitoring over 5 years reveals strong variations in the strength of the emission lines and for HD 45314 in the V/R ratio of the double-peaked emissions. Part of these long-term variations could be recurrent

Long-term Spectroscopic Variability of Two Oe Stars

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