Table 2:
Previous pulsation frequency determinations for HD 104237. The first column indicates the year of observation, the second column the frequency; the corresponding period is shown in Col. 3;
Col. 4 indicates spectroscopic or photometric oscillation amplitudes; the Col. 5 indicates the reference: [1] Donati et al. (1997), the 0.65 km s-1 amplitude in this table is calculated as half of the 1.3 km s-1 peak-to-peak amplitude stated in the paper; [2] Kurtz & Müller (2001).
Year |
Frequency |
Period |
Amplitude |
Reference |
|
(d-1) |
(min) |
|
|
1993 |
f1 = 37.3 |
38.6 |
0.65 km s-1 |
[1] |
1995 |
f1 = 39.6 |
36.4 |
0.65 km s-1 |
[1] |
1998 |
f1 = 33.29 |
43.3 |
11.2
0.5 mmag |
[2] |
|
f2 = 36.61 |
39.3 |
3.4
0.5 mmag |
[2] |
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