Table 3: Pulsating, irregular and cataclysmic variables. V is the minimum brightness for CVs and irregular, the mean brightness for pulsating variables. T0 is the time of maximum brightness for pulsating stars. Hereafter, the labels "k'' and "s'' indicate that the B-V color index is taken from Kaluzny & Rucinski (1995) or Stetson et al. (2003), respectively.

Star
Type $\alpha_{2000}$ $\delta_{2000}$ V $\langle B-V\rangle$ $\langle V-I\rangle$ Ref. T0 Period Ampl.
        [mag] [mag] [mag]   [HJD-2 452 400] [d] [mag]
Pulsating variables  
V123 HADS 19.362064 37.666034 17.08 0.45   k 59.559 0.06026 0.14
01497_12 HADS 19.379083 37.812419 16.06       59.528 0.07227 0.40
00311_7 SXPhe 19.324628 37.716768 23.17       59.605 0.10443 0.10
00224_10 SXPhe 19.353639 37.710163 21.72 0.71 1.06 s 59.801 0.12261 0.20
03653_3 RRc 19.347147 37.992413 17.21 0.57 0.58 k 59.937 0.32654 0.39
00345_1 RRab 19.325082 37.964170 18.28       60.151 0.57866 0.72

Irregular variables
 

V92
IRR 19.350754 37.766876 18.10 0.91   k     0.10
V83 IRR 19.346220 37.737232 19.10 1.02 1.05 k     0.07
V93 IRR 19.351452 37.785687 18.12 0.98 1.03 s     0.04

Cataclysmic variables
 

V15(=B7)
CV 19.352057 37.799019 18.26 0.20   k     0.06
B8 CV 19.343262 37.747833 20.64 -0.23 0.78 k     2.27
06289_9 CV (?) 19.348976 37.770355 22.80 0.25 0.88 s     3.10


Source LaTeX | All tables | In the text