- Table 1:
Characteristic velocity dispersions
in the thin
disk, thick disk, and stellar halo, used in
Eq. (1). X is the observed fraction of stars for
the populations in the solar neighbourhood and
asymmetric drift (values taken from Bensby et al. 2003 and
Bensby et al. submitted).
- Table 2:
Median ages and spreads for the sub-samples.
The first column gives the central
metallicity, and the second column the -enhancement.
Columns 3-6 give the following for the samples
the number of stars in the sub-sample,
the lower quartile for the age distribution, the median age,
and the upper quartile for the age distribution.
Columns 7-10 give the same information but for the samples