- ... galaxy
- Tables 1 and 4 are only available in electronic form at http://www.aanda.org
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... VLT/FLAMES
- Based on FLAMES observations collected at the European Southern Observatory, proposal 171.B-0588.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... observed
- Using different sets of isochrones, e.g.
Geneva (Lejeune & Schaerer 2001)
or Yonsei-Yale (Yi et al. 2001; Kim et al. 2002), would bring slightly different results, however qualitatively in
agreement.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...
population
- The velocity dispersion values we list are from the
weighted standard deviation and do not include the broadening due to measurement errors.
The true dispersion
is approximately
,
where
is the observed velocity dispersion and
is the average measured error in velocity. For our FLAMES data
the average error in velocity is
2 km s-1; the resulting values
of the velocity dispersion are thus only marginally inflated, for example if
km s-1 then
km s-1.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.