Up: On the origin of the O and B-type stars with high velocities
Appendix A: Distribution of differences
In this appendix we record the distribution of the difference between
two observables, each of which has a Gaussian error distribution.
We define two observable quantities, x1 and x2, which are both
distributed normally,
and
,
respectively, where
and
are the mean and standard deviation of G1, and
,
for G2. We define
as the
absolute difference between the observables, where
and
are the measurements of x1 and x2. We calculate the
distribution of the difference,
,
in the one-
(
), two-
(
), and three-dimensional
(
)
case. In all cases we took
and
and
.
The
former simplification is harmless since only the difference
is important. The results are:
![\begin{displaymath}F_{\rm 2D}(\Delta) = \frac{\Delta}{2 \sigma^2}
\exp \left [...
...^2} \right ]
I_0 \left (\frac{\Delta\mu}{2\sigma^2} \right ),
\end{displaymath}](/articles/aa/full/2001/02/aa10198/img368.gif) |
(A2) |
where I0 is a modified Bessel function of order zero, and
Applying L'Hospital's rule we calculate the limit of
for
:
![\begin{displaymath}\lim\limits_{\mu \rightarrow 0} F_{\rm 3D}(\Delta){\rm d}\Del...
...gma^3}
\exp \left [
- \frac{\Delta^2}{4\sigma^2}
\right ].
\end{displaymath}](/articles/aa/full/2001/02/aa10198/img373.gif) |
(A4) |
Figure A1 and Eqs. (A.2) and (A.3) show
that for the two- and three-dimensional cases there is a zero
probability of measuring the same value for x1 and x2, i.e.,
.
Up: On the origin of the O and B-type stars with high velocities
© ESO 2001