Table 3:
Possible rotational splittings for seven stars from our sample.
Designation of frequencies is the same as in Table 2.
|
Star |
 |
Splitting [d-1] |
Note |
| HD 74339 |
f3-f5 |
0.01690(4) |
quadruplet |
| |
f4-f3 |
0.01673(4) |
|
| |
f6-f4 |
0.01669(4) |
|
| HD 86214 |
f2-f5 |
0.00468(5) |
quadruplet |
| |
f3-f2 |
0.00505(4) |
|
| |
f4-f3 |
0.00495(4) |
|
| HD 94065 |
f5-f3 |
0.00155(4) |
triplet |
| |
f2-f5 |
0.00139(4) |
|
| HD 98260 |
f3-f2 |
0.03716(4) |
triplet |
| |
f1-f3 |
0.03386(4) |
|
| HD 168750 |
f3-f2 |
0.01833(2) |
triplet |
| |
f1-f3 |
0.01838(4) |
|
| HD 173502 |
f3-f4 |
0.17543(9) |
triplet |
| |
f1-f3 |
0.16308(3) |
|
| HD 186610 |
f1-f3 |
0.03871(4) |
triplet |
| |
f4-f1 |
0.03863(5) |
|
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