Issue |
A&A
Volume 561, January 2014
|
|
---|---|---|
Article Number | A84 | |
Number of page(s) | 17 | |
Section | Astrophysical processes | |
DOI | https://doi.org/10.1051/0004-6361/201322829 | |
Published online | 06 January 2014 |
Online material
Appendix A: Background and first-order contributions to the momentum influx
Here we evaluate Ṗ2 and Ṗ1, the
first two coefficients on the right-hand side of Eq. (55). We will show that both coefficients are zero. The first is
(A.1)Substituting
f2 = β sin θ/2
, this becomes
The
background flow, while it certainly carries z-momentum, makes no net
contribution to the influx.
The integral expression for the second coefficient is lengthier, and we write it as
(A.2)where
and
It
is convenient to split up the integral in Eq. (A.2) by region. For the downstream part, which we denote as
, we use
Eqs. (15) and (16) for f1 and
g-1. We find, after algebraic simplification, that
(A.3)We now use the identity
to conclude that (A.4)Similarly,
the upstream part is
(A.5)so
that
(A.6)For the intermediate
piece, to be denoted
, we use
Eqs. (21) and (22) for f1 and
g-1. Although we have established that
C = +1 , we will see that
is independent of
this parameter, so we retain the original notation. After algebraic manipulation, we
find
(A.7)Using the identity
we
infer that
(A.8)In
summary, we have
(A.9)
© ESO, 2014
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