Table 8.
Open in new tab

Best-fitting model for BPM 31594 considering all detected periods. The stellar mass, effective temperature, and hydrogen envelope are listed in column 2. The theoretical periods, harmonic degree, and radial order are listed in columns 3, 4, and 5, respectively. The value of the quality function is listed in the last row of column 2. The value of the rotation kernel is listed in the last column.

|$\#$|Π (s)ℓkCkℓ
M (M⊙)0.632315.2605210
Teff (K)11560406.339617
log (MH/M*)−4.12617.71961120.4825
χ21.5500644.1514113
679.0426114
1142.0466244
|$\#$|Π (s)ℓkCkℓ
M (M⊙)0.632315.2605210
Teff (K)11560406.339617
log (MH/M*)−4.12617.71961120.4825
χ21.5500644.1514113
679.0426114
1142.0466244
Table 8.
Open in new tab

Best-fitting model for BPM 31594 considering all detected periods. The stellar mass, effective temperature, and hydrogen envelope are listed in column 2. The theoretical periods, harmonic degree, and radial order are listed in columns 3, 4, and 5, respectively. The value of the quality function is listed in the last row of column 2. The value of the rotation kernel is listed in the last column.

|$\#$|Π (s)ℓkCkℓ
M (M⊙)0.632315.2605210
Teff (K)11560406.339617
log (MH/M*)−4.12617.71961120.4825
χ21.5500644.1514113
679.0426114
1142.0466244
|$\#$|Π (s)ℓkCkℓ
M (M⊙)0.632315.2605210
Teff (K)11560406.339617
log (MH/M*)−4.12617.71961120.4825
χ21.5500644.1514113
679.0426114
1142.0466244
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