![]() |
Figure 1: Observed R-parameter values as a function of the cluster [Fe/H] for the two adopted metallicity scales. The theoretical calibration for Y=0.245and a cluster age of 13 Gyr is also shown. |
Open with DEXTER |
![]() |
Figure 2:
He abundance values as a function of [Fe/H] for the 57 clusters analyzed. The two panels refer to the two metallicity scales
adopted in our analysis. The He abundances determined for the
clusters with [Fe/H] in the range comprised between the two vertical dotted
lines are affected by the choice of the cluster age. The
horizontal dashed line denotes
the most probable value for
![]() ![]() |
Open with DEXTER |
![]() |
Figure 3:
Probability Distribution Function (PDF) for
the He abundance in our GGC
sample when using the ZW84 metallicity scale. The dotted line
represents the PDF for the 51 clusters with [Fe/H] in the range not
affected by the cluster age (see text); the solid line represents the
subsample with
![]() ![]() |
Open with DEXTER |
![]() |
Figure 4: As in Fig. 3, but for the CG97 [Fe/H] scale (see text). |
Open with DEXTER |