000002024 001__ 2024
000002024 005__ 20160701171657.0
000002024 0247_ $$2DOI$$a10.1553/cia148s77
000002024 037__ $$aASTROimport-181
000002024 100__ $$aFrémat, Y.
000002024 245__ $$aSpectroscopy of HIP 113790 at the 5th OHP NEON summer school
000002024 260__ $$c2006
000002024 520__ $$aIn this contribution, we present the high-resolution observations we obtained for HIP 113790 at the Haute-Provence Observatory using the AURELIE spectrograph. By determing its fundamental parameters, we confirm that the star is located in the δ Scuti instability strip. We further report the detection of rapid line profile variations with a period of about 1.43 hours. 
000002024 700__ $$a Antonova, A.
000002024 700__ $$a Damerdji, Y.
000002024 700__ $$a Hansen, C. J.
000002024 700__ $$a Lederer, M. T.
000002024 700__ $$a Tüysüz, M.
000002024 700__ $$a Lampens, P.
000002024 700__ $$a van Cauteren, P.
000002024 773__ $$c77-81$$pCommunications in Asteroseismology$$v148$$y2006
000002024 85642 $$ahttp://esoads.eso.org/abs/2006CoAst.148...77F
000002024 905__ $$apublished in
000002024 980__ $$aREFERD