Astron. Astrophys. 326, 1001-1012 (1997)
Appendix A: species conservation
A.1. Mass fraction
Consider a species i whose mass fraction in the accreted
matter and in the star at shell j are
and , respectively. The total mass of element
i after accretion is given by and
represent a summation over the n shells of the model:
![[EQUATION]](img217.gif)
So, we have
![[EQUATION]](img218.gif)
and finally we obtain
![[EQUATION]](img219.gif)
A.2. Rescaled abundances
The new fractional mass derived alone
refers to the old mesh point. However, modifications of the mass
profile can result in changes in the mesh points. If k is the
shell number such that where subscript
j refers to the old mesh points and k to the current
ones, the interpolated composition at mass is
then
![[EQUATION]](img223.gif)
© European Southern Observatory (ESO) 1997
Online publication: April 8, 1998
helpdesk.link@springer.de  |