Adiabatic pulsation periods (up to 2000 sec) for g-modes with harmonic degree = 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*)

-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= 2 periods in a single file, please click here (12.7 Mb)