The interpretation of herd clusters was very similar for both breeds.
As was to be expected, the XP spectra of activated amino films corresponded to diamagnetic Ni II), showing that the concentration of Ni(OH 2 clusters was very small.
Another limitation was that our case definition for clusters was very specific.
Nonetheless, the number and the extent of GMYC clusters was very similar.
Even though differentiation among the new major clusters was very low (global FST = 0.005), stratification was still evident (λ = 1.19; calculated for the samples within the major clusters).
Severing in bare zones far from cofilin clusters was very rare.
However, in our study average cluster size was considerably lower than this, although the number of clusters was very large.
The identified members and the overall number of predicted clusters were very similar for both types of analyses, suggesting that the identification of clusters by these methods is relatively robust.
In both cases, the CRISPR-arrays located at each side of the cas gene clusters were very small (fig. 8).
Though proper motions of the clusters are very small, those for individual stars provide a useful criterion for cluster membership.
