Table A.1: 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.

Star
Type $\alpha_{2000}$ $\delta_{2000}$ V $\langle B-V\rangle$ $\langle V-I\rangle$ Ref. T0 Period Ampl. Memb. Distance
        [mag] [mag] [mag]   [HJD-2 452 400] [d] [mag]   [arcmin]
V123 HADS 19.362064 37.666034 17.08 0.45   k 59.559 0.06026 0.14 nm 11.8
01497_12 HADS 19.379083 37.812419 16.06       59.528 0.07227 0.40 nd2 22.2
00311_7 SXPhe 19.324628 37.716768 23.17       59.605 0.10443 0.10 nd2 17.0
00224_10 SXPhe 19.353639 37.710163 21.72 0.71 1.06 s 59.801 0.12261 0.20 nm 5.4
03653_3 RRc 19.347147 37.992413 17.21 0.57 0.58 k 59.937 0.32654 0.39 nm 13.3
00345_1 RRab 19.325082 37.964170 18.28       60.151 0.57866 0.72 nd2 20.0
V92 IRR 19.350754 37.766876 18.10 0.91   k     0.10 m 1.9
V83 IRR 19.346220 37.737232 19.10 1.02 1.05 k     0.07 m 2.4
V93 IRR 19.351452 37.785687 18.12 0.98 1.03 s     0.04 m 2.6
V15(=B7) CV 19.352057 37.799019 18.26 0.20   k     0.06 98 3.3
B8 CV 19.343262 37.747833 20.64 -0.23 0.78 k     2.27 m 3.7
06289_9 CV 19.348976 37.770355 22.80 0.25 0.88 s     3.10 m (B06) 0.7


Source LaTeX | All tables | In the text