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 |
 |
 |
V |
 |
 |
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