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. 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*) |
|||||||||||
|
|
|
|
|
|||||||
|
|
|
|||||||||
|
|||||||||||
|
|||||||||||
|
|||||||||||
|
|||||||||||
|