- ... Cepheids
- Based on observations collected at the European
Southern Observatory (La Silla, Chile) and at the
Observatoire de Haute-Provence (France).
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...1990)
- However, see Bono et al. (2000a) for a different interpretation.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... unweighted
- The nominal
uncertainties were not used, because the cross-correlation function for Cepheids is subject to large shape changes along
the pulsation cycle. These changes blur the relation between the computed uncertainty and the real velocity error.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.