Spectroscopy of HIP 113790 at the 5th OHP NEON summer school

Physics

Scientific paper

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Scientific paper

In this contribution, we present the high-resolution observations we obtained for HIP 113790 at the Haute-Provence Observatory using the AURELIE spectrograph. By determing its fundamental parameters, we confirm that the star is located in the δ Scuti instability strip. We further report the detection of rapid line profile variations with a period of about 1.43 hours.

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