Table 2: Physical parameters of the observing targets.

Stars		 Max.$ V^\dagger$ Var. type$^\dagger$ Sp. type$^\dagger$ P $_{\rm orb}$ ( day)$^\dagger$ Pulsation

TW Dra		 8.0 EA/SD A8V+K0III 2.806847 $P_{\rm pul}$ = 0 $.\!\!^{\rm d}$053, $\Delta$B $\approx$ 0 $.\!\!^{\rm m}$010
RX Hya 8.9 EA/SD A8 2.281645 $P_{\rm pul}$ = 0 $.\!\!^{\rm d}$052, $\Delta$B $\approx$ 0 $.\!\!^{\rm m}$014
AB Per 10.4 EA/SD A5 7.1602886 $P_{\rm pul}$ = 0 $.\!\!^{\rm d}$196, $\Delta$B $\approx$ 0 $.\!\!^{\rm m}$020
X Tri 8.55 EA/SD A5V+G0V 0.9715352 weak signals around 30 and 45 c/d ?
XZ UMa 10.1 EA/SD A5+F9 1.22232 -
AC UMa 10.3 EA/SD A2 6.854939 -
RW Per 9.68 EA/D A5IIIe+G0III 13.198904 -
ST Per 9.52 EA/SD A3V+G 2.648315 -
RV Per 10.3 EA/SD A2 1.9734926 -
CP And 11.4 EA/SD A5 3.60894 -
VZ Leo 11.8 EA/SD A5 1.089906 -
RS Cep 10.2 EA/SD A5IIIe+G 12.420105 -
Z Dra 10.8 EA/SD F4V 1.357456 -
RW CrB 10.2 EA/SD F2V 0.7264114 -
$^\dagger$ From the GCVS (Kholopov et al. 1988).    


Source LaTeX | All tables | In the text