Table 6.

Potential best-fitting models for each set of the periods considered for G 29 − 38.

Teff (K)log gMWD/MMH/MWDMHe/MWDℓ = 1χd[pc]
K9811 5778.040.6327.58 × 10−051.74 × 10−0293.7417.45
T0811 4468.220.7215.64 × 10−107.25 × 10−0343.2415.30
TESS11 6358.040.6327.58 × 10−051.74 × 10−02154.7217.54
TESS+K98 + T0811 6208.390.8373.91 × 10−063.18 × 10−03154.3613.66
11 6358.040.6327.58 × 10−051.74 × 10−02154.8617.54
Teff (K)log gMWD/MMH/MWDMHe/MWDℓ = 1χd[pc]
K9811 5778.040.6327.58 × 10−051.74 × 10−0293.7417.45
T0811 4468.220.7215.64 × 10−107.25 × 10−0343.2415.30
TESS11 6358.040.6327.58 × 10−051.74 × 10−02154.7217.54
TESS+K98 + T0811 6208.390.8373.91 × 10−063.18 × 10−03154.3613.66
11 6358.040.6327.58 × 10−051.74 × 10−02154.8617.54

Together with the basic stellar parameters, we list the number of pulsation periods associated with ℓ = 1 modes, the value of the quality function χ, and the asteroseismic distance.

Table 6.

Potential best-fitting models for each set of the periods considered for G 29 − 38.

Teff (K)log gMWD/MMH/MWDMHe/MWDℓ = 1χd[pc]
K9811 5778.040.6327.58 × 10−051.74 × 10−0293.7417.45
T0811 4468.220.7215.64 × 10−107.25 × 10−0343.2415.30
TESS11 6358.040.6327.58 × 10−051.74 × 10−02154.7217.54
TESS+K98 + T0811 6208.390.8373.91 × 10−063.18 × 10−03154.3613.66
11 6358.040.6327.58 × 10−051.74 × 10−02154.8617.54
Teff (K)log gMWD/MMH/MWDMHe/MWDℓ = 1χd[pc]
K9811 5778.040.6327.58 × 10−051.74 × 10−0293.7417.45
T0811 4468.220.7215.64 × 10−107.25 × 10−0343.2415.30
TESS11 6358.040.6327.58 × 10−051.74 × 10−02154.7217.54
TESS+K98 + T0811 6208.390.8373.91 × 10−063.18 × 10−03154.3613.66
11 6358.040.6327.58 × 10−051.74 × 10−02154.8617.54

Together with the basic stellar parameters, we list the number of pulsation periods associated with ℓ = 1 modes, the value of the quality function χ, and the asteroseismic distance.

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