000002285 001__ 2285
000002285 005__ 20160701171702.0
000002285 0247_ $$2DOI$$a10.1007/s10509-009-0219-z
000002285 037__ $$aASTROimport-442
000002285 100__ $$aMaisonneuve, F.
000002285 245__ $$aSpectroscopic mode identification of main-sequence non-radially pulsating stars
000002285 260__ $$c2010
000002285 520__ $$aWe are undertaking an extensive observational campaign of a number of non-radially pulsating stars using the high-resolution HERCULES spectrograph on the 1.0-m telescope at the Mt John University Observatory. This is part of a large world-wide multi-site campaign to improve mode-identification techniques in non-radially pulsating stars, particularly for g-mode pulsators. This paper outlines our campaign and presents preliminary results for one γ Doradus star, HD 40745, and one β Cephei star, HD 61068. We have used a representative cross-correlation line-profile technique presented by Wright in 2008 to extract line profiles and these have then been analyzed using the FAMIAS package due to Zima published in 2006 to derive a spectroscopic mode identification. 
000002285 700__ $$a Pollard, K. R.
000002285 700__ $$a Cottrell, P. L.
000002285 700__ $$a Kilmartin, P. M.
000002285 700__ $$a Wright, D. J.
000002285 700__ $$a De Cat, P.
000002285 773__ $$c105-108$$i1-2$$pAstrophysics and Space Science$$v328$$y2010
000002285 85642 $$ahttp://esoads.eso.org/abs/2010Ap%26SS.328..105M
000002285 905__ $$apublished in
000002285 980__ $$aREFERD