Adiabatic
pulsation periods (up to 2000 sec) for g-modes with harmonic degree
ℓ=
1 (dipole
modes)
Below,
values of the stellar mass of our set of DA white dwarf models are
in the upper row, and the mass of H corresponding to the different
envelope thicknesses considered for each stellar mass are in rows 2
to 9. In particular, row 2 shows the maximum value of the thickness
of the H envelope (“canonical envelope thickness”) for
each stellar mass according to our evolutionary computations. You
can download a specific set of files containing pulsation periods,
forward period spacings, time averaged oscillation kinetic energies,
and first order rotational splitting coefficients by simply clicking
on a given element of the table associated to a DA white dwarf
sequence. For details, see Romero,
Córsico, Althaus et al. (2012).
M*/Mo
|
0,5249
|
0,5480
|
0,5701
|
0,5932
|
0,6096
|
0,6323
|
0,6598
|
0,7051
|
0,7670
|
0,8373
|
0,8779
|
log(MH/M*)
|
-3.62
|
-3.74
|
-3.82
|
-3.93
|
-4.02
|
-4.12
|
-4.25
|
-4.45
|
-4.7
|
-5
|
-5.07
|
|
-4.27
|
-4.27
|
-4.28
|
-4.28
|
-4.45
|
-4.46
|
-4.59
|
|
|
|
|
|
-4.85
|
-4.85
|
-4.84
|
-4.85
|
-4.85
|
-4.86
|
-4.87
|
-4.88
|
-4.91
|
|
|
|
-5.35
|
-5.35
|
-5.34
|
-5.34
|
-5.35
|
-5.35
|
-5.35
|
-5.36
|
-5.37
|
-5.41
|
-5.4
|
|
-6.33
|
-6.35
|
-6.33
|
-6.33
|
-6.34
|
-6.34
|
-6.35
|
-6.35
|
-6.36
|
-6.36
|
-6.39
|
|
-7.34
|
-7.33
|
-7.34
|
-7.34
|
-7.33
|
-7.35
|
-7.33
|
-7.35
|
-7.34
|
-7.36
|
-7.38
|
|
-8.33
|
-8.33
|
-8.31
|
-8.33
|
-8.33
|
-8.33
|
-8.33
|
-8.34
|
-8.33
|
-8.34
|
-8.37
|
|
-9.25
|
-9.22
|
-9.33
|
-9.33
|
-9.25
|
-9.34
|
-9.33
|
-9.34
|
-9.33
|
-9.34
|
-9.29
|
If
you want to download the complete set of ℓ= 1
periods
in a single file, please click here
(7.6
Mb)