Time-Resolved Halpha Monitoring of the Herbig Ae/Be Star HD 200775

Computer Science

Scientific paper

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Young Variable Stars, Spectral Variability

Scientific paper

Our time-resolved H_alpha monitoring of V380 Cep has revealed no
significant rapid profile variations for the components of the H_alpha
line. A slow shift to shorter wavelengths of individual line components
was observed during 20 days. The results are difficult to interpret as
resulting from the star's axial rotation.

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