
Figure 28: Accreted mass as a function of the accretion rate for models experiencing a dynamical
He-flash. The lines refer to WD with different initial masses — 0.6, 0.7, 0.81, 0.92, 1.02
.
Piersanti, Tornambé and Yungelson in prep.
.
Piersanti, Tornambé and Yungelson in prep.
