Table 3.

The explored parameter spaces of WDs evolved by wdec.

ParametersInitial rangesCrude stepsFine stepsOptimal valuesaOptimal valuesb
M*/M[0.500, 0.850]0.0100.0050.760 ± 0.0050.690 ± 0.005
Teff(K)[10 600, 12 600]2501012110 ± 1012370 ± 10
log(Menv/M*)[1.50, 2.00, 3.00]0.50/1.000.012.00 ± 0.023.00 ± 0.01
log(MHe/M*)[2.00, 5.00]1.000.015.01 ± 0.044.99 ± 0.01
log(MH/M*)[4.00, 10.00]1.000.019.98 ± 0.027.00 ± 0.01
XHe in mixed C/He/H region[0.10, 0.90]0.160.010.25 ± 0.010.56 ± 0.01
XO in the core
h1[0.60, 0.75]0.030.010.73 ± 0.010.66 ± 0.01
h2[0.65, 0.71]0.030.010.66 ± 0.010.71 ± 0.01
h30.85 –0.010.81 ± 0.030.85 ± 0.01
w1[0.32, 0.38]0.030.010.35 ± 0.010.37 ± 0.01
w2[0.42, 0.48]0.030.010.45 ± 0.010.46 ± 0.01
w30.09 –0.010.09 ± 0.010.12 ± 0.01
ParametersInitial rangesCrude stepsFine stepsOptimal valuesaOptimal valuesb
M*/M[0.500, 0.850]0.0100.0050.760 ± 0.0050.690 ± 0.005
Teff(K)[10 600, 12 600]2501012110 ± 1012370 ± 10
log(Menv/M*)[1.50, 2.00, 3.00]0.50/1.000.012.00 ± 0.023.00 ± 0.01
log(MHe/M*)[2.00, 5.00]1.000.015.01 ± 0.044.99 ± 0.01
log(MH/M*)[4.00, 10.00]1.000.019.98 ± 0.027.00 ± 0.01
XHe in mixed C/He/H region[0.10, 0.90]0.160.010.25 ± 0.010.56 ± 0.01
XO in the core
h1[0.60, 0.75]0.030.010.73 ± 0.010.66 ± 0.01
h2[0.65, 0.71]0.030.010.66 ± 0.010.71 ± 0.01
h30.85 –0.010.81 ± 0.030.85 ± 0.01
w1[0.32, 0.38]0.030.010.35 ± 0.010.37 ± 0.01
w2[0.42, 0.48]0.030.010.45 ± 0.010.46 ± 0.01
w30.09 –0.010.09 ± 0.010.12 ± 0.01

Notes. M* denotes the stellar mass, while Menv is the envelop mass. MH is the mass of hydrogen atmosphere, and MHe is the mass of He layer. XHe is the He abundance in the mixed C/He/H region, and XO is the O abundance in the core. The parameter h1 refers to the O abundance in the core centre, while w1 is the mass fraction of XO = h1. Parameters h2 and h3 are O abundance of two knee points on the reducing O profile. The w2 and w3 refer to the masses of the gradient regions of O profile.

a

Adopted solution.

b

Additional solution found by freeing the value of l.

Table 3.

The explored parameter spaces of WDs evolved by wdec.

ParametersInitial rangesCrude stepsFine stepsOptimal valuesaOptimal valuesb
M*/M[0.500, 0.850]0.0100.0050.760 ± 0.0050.690 ± 0.005
Teff(K)[10 600, 12 600]2501012110 ± 1012370 ± 10
log(Menv/M*)[1.50, 2.00, 3.00]0.50/1.000.012.00 ± 0.023.00 ± 0.01
log(MHe/M*)[2.00, 5.00]1.000.015.01 ± 0.044.99 ± 0.01
log(MH/M*)[4.00, 10.00]1.000.019.98 ± 0.027.00 ± 0.01
XHe in mixed C/He/H region[0.10, 0.90]0.160.010.25 ± 0.010.56 ± 0.01
XO in the core
h1[0.60, 0.75]0.030.010.73 ± 0.010.66 ± 0.01
h2[0.65, 0.71]0.030.010.66 ± 0.010.71 ± 0.01
h30.85 –0.010.81 ± 0.030.85 ± 0.01
w1[0.32, 0.38]0.030.010.35 ± 0.010.37 ± 0.01
w2[0.42, 0.48]0.030.010.45 ± 0.010.46 ± 0.01
w30.09 –0.010.09 ± 0.010.12 ± 0.01
ParametersInitial rangesCrude stepsFine stepsOptimal valuesaOptimal valuesb
M*/M[0.500, 0.850]0.0100.0050.760 ± 0.0050.690 ± 0.005
Teff(K)[10 600, 12 600]2501012110 ± 1012370 ± 10
log(Menv/M*)[1.50, 2.00, 3.00]0.50/1.000.012.00 ± 0.023.00 ± 0.01
log(MHe/M*)[2.00, 5.00]1.000.015.01 ± 0.044.99 ± 0.01
log(MH/M*)[4.00, 10.00]1.000.019.98 ± 0.027.00 ± 0.01
XHe in mixed C/He/H region[0.10, 0.90]0.160.010.25 ± 0.010.56 ± 0.01
XO in the core
h1[0.60, 0.75]0.030.010.73 ± 0.010.66 ± 0.01
h2[0.65, 0.71]0.030.010.66 ± 0.010.71 ± 0.01
h30.85 –0.010.81 ± 0.030.85 ± 0.01
w1[0.32, 0.38]0.030.010.35 ± 0.010.37 ± 0.01
w2[0.42, 0.48]0.030.010.45 ± 0.010.46 ± 0.01
w30.09 –0.010.09 ± 0.010.12 ± 0.01

Notes. M* denotes the stellar mass, while Menv is the envelop mass. MH is the mass of hydrogen atmosphere, and MHe is the mass of He layer. XHe is the He abundance in the mixed C/He/H region, and XO is the O abundance in the core. The parameter h1 refers to the O abundance in the core centre, while w1 is the mass fraction of XO = h1. Parameters h2 and h3 are O abundance of two knee points on the reducing O profile. The w2 and w3 refer to the masses of the gradient regions of O profile.

a

Adopted solution.

b

Additional solution found by freeing the value of l.

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