Table 2: Data on the programme stars. Spectral type are taken from SIMBAD and WEBDA online database. $T_{\rm {eff}}$ and $\log g$ are those determined by UVBYBETA code. $v_{\rm e}\sin i$ and $\xi _{t}$ are determined as explained in Sect. 3.2.1. References (a) and (b) are Bounatiro (1993) and Rodriguez et al. (1994) respectively.
TR HD Type mv $T_{\rm {eff}}$ $\log g$ $v_{\rm e}\sin i$ $\xi _{t}$ Remarques
        (K)   km s-1 km s-1  
19 HD 106103 F5V 8.09 6707 4.45 19.7 1.4  
  HD 106293 F5V 8.09 6545 4.34 47 1.4  
36 HD 106691 F5IV 8.08 6713 4.43 37 1.6  
49 HD 106946 F2V 7.87 6892 4.30 62 1.9  
86 HD 107611 F6V 8.50 6491 4.57 22 1.4  
  HD 109530 F2V 7.30 6497 3.85 67 2.1  
101 HD 107877 F6 8.35 6598 4.54 29.5 1.25  
114 HD 108154 F5 8.56 6497 4.54 19 1.15  
118 HD 108226 F5 8.34 6530 4.45 19 1.05  
162 HD 108976 F6 V 8.54 6413 4.49 20 1.1  
  HD 109069 F0 V 7.55 6864 4.06 89 2.2  
107 HD 107966 A3V/A3IV 5.18 8541 3.82 51 2.9  
130 HD 108382 A4V/A3IV 4.96 8317 3.92 75.5 3.2  
47 HD 106887 A4m 5.71 8291 4.20 82 3.8  
86 HD 107655 A0V 6.18 9675 4.10 45 2.0 $\notin$ Coma (a)
62 HD 107168 A8m/kA5hA5mF0 6.24 8283 4.20 14.3 4.0  
183 HD 109307 A4Vm/A3IV-V 6.26 8396 4.10 14.5 3.3  
144 HD 108642 A2m/kA2hA7mA7 6.54 8079 4.06 9.2 3.7  
68 HD 107276 Am/Ka5mA7 6.63 8000 4.00 102 2.8  
139 HD 108486 AmkA3hA5mA7 6.67 8148 4.11 37 3.0  
52 HD 106999 Am 7.46 8148 4.09 44 3.0 $\notin$ Coma (a)
82 HD 107513 Am/kA7hF0mF0 7.38 7279 4.02 62 3.0 $\delta$ Scuti (b)

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