All Figures

	Figure 1: Phase diagram of the radial velocity ( top left) and the Hipparcos measurements ( bottom left) of HD 34025 with the period as given in the bottom right corner. The reference epoch is HJD 2450000. The dashed lines in the bottom left panel denote the phase at which  = . In the right panel, a selection of observed cross-correlation profiles are shown as a function of orbital phase.
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In the text

	Figure 4: Same as Fig. 1, but for HD 85964.
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In the text

	Figure 5: Same as Fig. 1, but for HD 10167.
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In the text

	Figure 7: Same as Fig. 1, but for HD 126516.
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In the text

	Figure 11: Phase diagrams for the intrinsic periods of HD 209295 found in the residual dataafter prewhitening with the orbit given in Table 3. The reference epoch is HJD 2450000. Top left: P 1 = 0.4343(2) d. Top right: P 2 = 0.8853(9) d (prewhitened with P 1). Bottom left: P 3 = 0.8535(9) d (prewhitened with P 1). Bottom right: P 4 = 0.3882(2) d (prewhitened with P 1, P 2 and P 3).
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In the text

	Figure 12: Phase diagram of the radial velocity (top left) and the Hipparcos measurements (bottom left) of HD 40745 with the period as given in the bottom right corner. The reference epoch is HJD 2450000. In the right panel, a selection of observed cross-correlation profiles are shown as a function of pulsation phase.
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In the text

	Figure 19: Phase diagram of the radial velocity with our best fitting period ( top left) and the best fitting photometric period ( bottom left) of HD 14940. The period values are given in the bottom right corner. The reference epoch is HJD 2 450 000. In the right panel, a selection of observed cross-correlation profiles are shown as a function of our best fitting period.
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In the text

	Figure 20: Same as Fig. 19, but for HD 27290.
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In the text

Figure 25: Comparison of the values (full circles with error boxes) determined with the Fourier method ( ) to those determined by a least-square fitting with synthetic profiles ( ). The components known to be pulsating are given in blue, and those for which the value is only based on 1 cross-correlation profile are given in red. The colour representation is only available in the online version of the paper.

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In the text

Figure 26: Histograms showing the number of bf  Dor stars ( ; top), cand  Dor stars ( ; middle), and rejected  Dor stars that were formerly under consideration ( ; bottom) as a function of . The values from this work are given in dark grey. The other values were taken from Henry & Fekel (2005); Handler (2002); Henry & Fekel (2002); Henry et al. (2005); Fekel et al. (2003); Mathias et al. (2004); Henry & Fekel (2003).

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In the text

	Figure 2: Same as Fig. 1, but for HD 81421.
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In the text

	Figure 3: Same as Fig. 1, but for HD 214291.
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In the text

	Figure 6: Same as Fig. 1, but for HD 147787. The dotted line in the top left panel indicates the time of periastron passage.
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In the text

	Figure 8: Same as Fig. 1, but for HD 167858. In the top panel, the radial velocities, as determined by Fekel & Henry (2003), are included and given in grey.
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In the text

	Figure 9: Same as Fig. 1, but for HD 209295. The dotted line in the top left panel indicates the time of periastron passage.
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In the text

Figure 10: The cross-correlation profiles of the observed CORALIE spectra for the (suspected) binary objects for which no orbital solution could be determined with our current set of CORALIE data. Subsequent profiles are shifted in flux for clarity. The name of the object and the orbital classification are given at the top of each panel. "SB2'', "SB1'', "VB'', and "ellipsoidal'' indicate double-lined binaries, single-lined binaries, visual binaries, and ellipsoidal variables, respectively.

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In the text

	Figure 13: Same as Fig. 12, but for HD 41448.
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In the text

	Figure 14: Same as Fig. 12, but for HD 112685.
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In the text

	Figure 15: Same as Fig. 12, but for HD 187028.
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In the text

	Figure 16: Same as Fig. 12, but for HD 125081.
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In the text

	Figure 17: Same as Fig. 12, but for HD 135825.
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In the text

	Figure 18: Same as Fig. 12, but for HD 218225.
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In the text

	Figure 21: Phase diagrams of the radial velocity with two known HIPPARCOS periods of HD 149989 ( left). The period values are given in the bottom right corner. The reference epoch is HJD 2450000. In the right panel, a selection of observed cross-correlation profiles are shown as a function of the main HIPPARCOS period.
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In the text

	Figure 22: Same as Fig. 21, but for HD 216910.
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In the text

	Figure 23: The cross-correlation profiles of the observed CORALIE spectra for HD 65526. Subsequent profiles are shifted in flux for clarity.
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In the text

	Figure 24: The cross-correlation profiles of the observed CORALIE spectra for the objects for which no clear correlation profile variations have been detected in our current set of CORALIE data. Subsequent profiles are shifted in flux for clarity. The HD number of the object is given at the top of each panel.
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In the text