Adiabatic pulsation periods (up to 2000 sec) for g-modes with harmonic degree ℓ= 2 (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*) |
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If you want to download the complete set of ℓ= 2 periods in a single file, please click here (12.7 Mb)