Table 3:
The results for 
Bootis stars taken from Paunzen et al. (2002)
according to Fig. 1 and Table 2.
We would only consider the stars of group (5)
as good candidates for undetected spectroscopic binary systems, and
no conclusion can be drawn for group (6).
| (1) |
(2) |
( 3 ) |
(4) |
(5) |
( 6 ) a. |
| 6870 |
319 |
31295 |
111604 |
23392 |
13755 P |
| 11413 |
7908 |
35242 |
156954 |
110377 |
15165 P |
| 24472 |
30422 |
101108 |
193256 |
170680 |
54272 P |
| 75654 |
74873 |
|
193281 |
198160 |
87271 P |
| 81290 |
91130 |
|
|
|
90821 F |
| 83041 |
110411 |
|
|
|
105759 P |
| 83277 |
125162 |
|
|
|
111005 P |
| 84123 |
130767 |
|
|
|
120500 F |
| 102541 |
183324 |
|
|
|
120896 P |
| 105058 |
204041 |
|
|
|
175445 F |
| 106223 |
221756 |
|
|
|
|
| 107233 |
|
|
|
|
|
| 109738 |
|
|
|
|
|
| 125889 |
|
|
|
|
|
| 142703 |
|
|
|
|
|
| 142994 |
|
|
|
|
|
| 149130 |
|
|
|
|
|
| 153747 |
|
|
|
|
|
| 154153 |
|
|
|
|
|
| 168740 |
|
|
|
|
|
| 168947 |
|
|
|
|
|
| 184779 |
|
|
|
|
|
| 192640 |
|
|
|
|
|
| 210111 |
|
|
|
|
|
| 216847 |
|
|
|
|
|
| 44% |
19% |
5% |
7% |
7% |
18% |
|
a. Passed (intrinsic Bootis ) or Failed (undetected
binary system); The last row contains the percentage
of objects as part of the total sample.
|
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