Table 1: Overview of the 37 targets discussed in this paper. For each object, we give: the HD number (1), the HIPPARCOS number (2), the Johnson V magnitude (3) and the spectral classification (4) as found in the SIMBAD astronomical database; the number of CORALIE spectra (5) and their total time span expressed in days (6); the main HIPPARCOS period in days (7); the orbital classification (8); an indication of the observation of cross-correlation profile variations (9); the variability classification (10); and the mean $v \sin i$ values obtained by least-square fitting with synthetic profiles for the primary (11) and secondary (12) components. The errors are given between brackets in units of the last decimal. The targets that are in common with those of the Eyer et al. sample (in preparation) are indicated by $\ast $ in Col. (1). The stars that were already classified as confirmed or suspected binaries are indicated by + in Col. (8). The stars already classified as bf $\gamma $ Dor stars are indicated by $\hbox {$^\circ $ }$ in Col. (10).
HD HIP mV SpT $\char93 $ $\Delta T$ $P _{\rm hipp}$   binarity CPVs variability $v \sin i$
    (mag)     (days) (days)         (km$\;$s-1)
(1) (2) (3) (4) (5) (6) (7)   (8) (9) (10) (11) (12)
5590 4481 9.21 F2 V 16 1355     SB2   constant 103(3) 3.4(0.3)
7455 5745 8.47 G3 V 19 1723       no constant 3.3(3)  
8393 6387 9.49 F7w 14 1136     SB2   constant 4.1(3) 3.7(2)
10167$\ast $ 7649 6.67 F0 V 15 1721     SB2+   cand $\gamma $ Dor 4.5(5) 4.9(6)
12901$\ast $ 9807 6.74 F0 50 1721 2.18: [2]   yes bf $\gamma $ Dor $\hbox {$^\circ $ }$ 64(3)  
14940$\ast $ 11192 6.68 F0 IV/V 63 685 0.50038 [1]   yes bf $\gamma $ Dor 39(4)  
22001 16245 4.71 F5 IV/V 18 1719       no constant 12(2)  
26298$\ast $ 19383 8.16 F0/F2 V 9 332     SB1?   cand $\gamma $ Dor? 50.9(5)  
27290 19893 4.26 F4 III 19 1395 0.757031 [1]   yes bf $\gamma $ Dor $\hbox {$^\circ $ }$(/$\delta$ Sct?) 55(2)  
27377$\ast $ 20036 7.4 F0 V 3 13 2.8482 [3] SB2   cand $\gamma $ Dor? 5.5(4) 5.2(6)
27604 20109 6.08 F7 IV/V 3 6     VB?   constant 67.5(4) 4.3(3)
33262 23693 4.71 F7 V 19 1722 0.28603 [3]   no constant 10.1(10)  
34025$\ast $ 24215 7.87 F2 IV 8 302 0.62221 [1] SB2 yes bf $\gamma $ Dor 62.8(11) 39(2)
35416$\ast $ 25183 7.53 F3 V 11 625     SB2   cand $\gamma $ Dor? 6.6(?) 6.0(?)
40745$\ast $ 28434 6.21 F2 IV 8 334 0.82415 [1]   yes bf $\gamma $ Dor 39(2)  
41448$\ast $ 28778 7.60 A9 V 12 10 0.419912 [1]   yes bf $\gamma $ Dor 106(3)  
48501$\ast $ 32144 6.26 F2 V 34 1493       yes bf $\gamma $ Dor $\hbox {$^\circ $ }$ 44(4)  
65526$\ast $ 39017 6.98 A3 2 1 1.28798 [1]   yes bf $\gamma $ Dor $\hbox {$^\circ $ }$ 56(4)  
81421$\ast $ 46223 7.01 A3 63 384 0.489724 [1] SB2+   constant 62.0(4) 42(4)
85964$\ast $ 48580 7.52 F3 IV/V 11 381 0.62425 [1] SB1   constant 65(2)  
110379   3.65 F0 V 8 15         cand $\gamma $ Dor 23.9(6)  
110606$\ast $ 62105 7.8 F2 V 7 75 0.977 [2] SB2+   cand $\gamma $ Dor 5.8(4) 10(2)
111709$\ast $ 62774 9.27 A3:m... 5 78 1.18567 [1] SB2 yes cand $\gamma $ Dor/CP star? 61(1) 25(4)
111829$\ast $   9.49 A1 IV/V 2 0     SB2?   cand $\gamma $ Dor? 47(2) ?
112685$\ast $ 63372 7.85 F0 V 24 385 0.61645 [1]   yes bf $\gamma $ Dor 70(3)  
112934$\ast $ 63491 6.6 A9 V 5 79 0.8: [2]     cand $\gamma $ Dor 70.5(7)  
125081$\ast $ 69848 7.35 F2 II 7 77 0.153981 [1]   yes bf $\delta$ Sct 5.6(5)  
126516$\ast $ 70566 8.2 F3 V 9 76 0.493 [2] SB1+   cand $\gamma $ Dor 3.8(3)  
135825$\ast $ 74825 7.31 F0 17 450 0.76053 [1]   yes bf $\gamma $ Dor 38(5)  
147787$\ast $ 80645 5.28 F4 IV 10 377 1.45557 [1] SB2+   cand $\gamma $ Dor 7.6(?) 25(?)
149989$\ast $ 81650 6.30 A9 V 10 379 0.42658 [1]   yes bf $\gamma $ Dor 134(3)  
167858$\ast $ 89601 6.62 F2 V 7 3 1.30700 [1] SB1+   bf $\gamma $ Dor $\hbox {$^\circ $ }$ 5.0(2)  
187028$\ast $ 97590 7.60 F0 V 21 179 0.69532 [1]   yes bf $\gamma $ Dor 85(3)  
209295$\ast $ 108976 7.5 A9/F0 V 61 1399 0.885274 [1] SB1+ yes bf $\gamma $ Dor/$\delta$ Sct $\hbox {$^\circ $ }$ 86(3)  
214291 111718 6.54 F7 V 5 1329 0.87125 [1] SB2+   cand $\gamma $ Dor? 67.6(8) 64.7(7)
216910$\ast $ 113402 6.70 F2 IV 11 1718 0.69349 [1]   yes bf $\gamma $ Dor 92(3)  
218225$\ast $ 114127 8.72 F3 IV 14 1327 0.86679 [1]   yes bf $\gamma $ Dor 59(3)  
$\textstyle \parbox{17cm}{ {[1] \citet{ESA1997}; [2] \citet{Handler1999MNRAS.309L..19H}; [3] \citet{Koen2002MNRAS.331...45K}}.}$

Source LaTeX | All tables | In the text