2024 20160701171657.0 10.1553/cia148s77 DOI ASTROimport-181 Frémat, Y. 2006 Spectroscopy of HIP 113790 at the 5th OHP NEON summer school 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. Antonova, A. Damerdji, Y. Hansen, C. J. Lederer, M. T. Tüysüz, M. Lampens, P. van Cauteren, P. Communications in Asteroseismology 148 2006 77-81 http://esoads.eso.org/abs/2006CoAst.148...77F published in REFERD