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2006CoAst.148...77F - Com. in Asteroseismology, 148, 77 (2006/December-0)
Spectroscopy of HIP 113790 at the 5th OHP NEON summer school.
FREMAT Y., ANTONOVA A., DAMERDJI Y., HANSEN C.J., LEDERER M.T., TUYSUZ M., LAMPENS P. and VAN CAUTEREN P.
Abstract (from CDS):
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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Simbad objects: 1
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