000001971 001__ 1971
000001971 005__ 20160701171656.0
000001971 037__ $$aASTROimport-128
000001971 100__ $$aWright, D. J.
000001971 245__ $$aRotation and pulsation in g-mode main sequence pulsators
000001971 260__ $$c2008
000001971 520__ $$aThe lack of well-identified modes is one of the major problems preventing an in-depth as- teroseismic study of gravity-mode (g-mode) main sequence pulsators. Since several of the currently available spectroscopic mode identification techniques have been developed for, or only extensively tested on pressure-mode pulsations, we started an investigation to improve them for the high radial order g-modes observed for slowly pulsating B (SPB) and γ Doradus (γ Dor) stars. A few high quality spectroscopic timeseries are being obtained for a selection of the most promising members of these groups with a large spread in projected rotational velocity that will serve as testbeds. These data will also enable us to study any observational relationship between the observed g-modes (degree l, azimuthal number m and/or pulsation amplitude) and the rotation of these non-radially pulsating stars. 
000001971 700__ $$a De Cat, P.
000001971 700__ $$a Pollard, K. R.
000001971 700__ $$a Zima, W.
000001971 773__ $$c383-384$$pCommunications in Asteroseismology$$v157$$y2008
000001971 85642 $$ahttp://esoads.eso.org/abs/2008CoAst.157..383W
000001971 905__ $$apublished in
000001971 980__ $$aREFERD