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000002216 0247_ $$2DOI$$a10.1111/j.1365-2966.2012.20861.x
000002216 037__ $$aASTROimport-373
000002216 100__ $$aBrunsden, E.
000002216 245__ $$aSpectroscopic pulsational frequency identification and mode determination of γ Doradus star HD 135825
000002216 260__ $$c2012
000002216 520__ $$aWe present the mode identification of frequencies found in spectroscopic observations of the γ Doradus star HD 135825. Four frequencies were successfully identified: 1.3150 ± 0.0003, 0.2902 ± 0.0004, 1.4045 ± 0.0005 and 1.8829 ± 0.0005 d-1. These correspond to (l, m) modes of (1, 1), (2, -2), (4, 0) and (1, 1), respectively. Additional frequencies were found but they were below the signal-to-noise ratio limit of the Fourier spectrum and not suitable for mode identification. The rotational axis inclination and v sin i of the star were determined to be 87° (nearly edge-on) and 39.7 km s-1 (moderate for γ Doradus stars), respectively. A simultaneous fit of these four modes to the line profile variations in the data gives a reduced χ2 of 12.7. We confirm, based on the frequencies found, that HD 135825 is a bona fide γ Doradus star. 
000002216 700__ $$a Pollard, K. R.
000002216 700__ $$a Cottrell, P. L.
000002216 700__ $$a Wright, D. J.
000002216 700__ $$a De Cat, P.
000002216 700__ $$a Kilmartin, P. M.
000002216 773__ $$c3535-3545$$i4$$pMonthly Notices of the Royal Astronomical Society$$v422$$y2012
000002216 85642 $$ahttp://esoads.eso.org/abs/2012MNRAS.422.3535B
000002216 905__ $$apublished in
000002216 980__ $$aREFERD