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The clusters are very large, with diameters measuring from 10 to as much as 300 light-years.
The study on structure property relationships of polynuclear 3d-Gd clusters are very essential in the fields of magnetic refrigerants.
Though proper motions of the clusters are very small, those for individual stars provide a useful criterion for cluster membership.
The large carbon clusters are very stable compounds with the respect to various physical and chemical factors.
Apart from aiding the development of novel materials, clusters are very useful for understanding the intrinsic and fundamental nature of molecular recognition and self-assembling phenomena.
The residual magnetism and coercivity of clusters are very low.
Similar(22)
In addition, performance comparison with conventional parallel computers and PC clusters is very cumbersome or impossible since the latter often employ MPI or similar communication libraries.
Besides the expected uniqueness of the Gly and Pro distributions, the nonpolar/β-branched and AsX clusters were very consistent across all types of secondary structure.
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.
Complete aerodynamic dispersion of cohesive clusters is very challenging to achieve, due to large interparticle attractive forces compared to dispersive forces.
Effect of basis set on the fragmentation energy of clusters is very little, but similar trend is observed for different basis set nevertheless.
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