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| | CHAPTER 8 |
 | | As in the star cluster, the resu It is an eyuilibrium between the inward motion of the outer particles and the outward motion of the inner particles. |
 | | Furthermore, the HR diagram of this cluster, which indicates its stellar composition, is almost identical with that of a late type globular cluster, such as M 13, whereas the stars of the open clusters that are now seen to be older, are mainly main sequence stars, comparable to the general population in their environment. |
 | | As the clusters are pulled slowly in toward the Galaxy gravitationally, the atombuilding processes that are under way in all matter inerease the proportion of heavy elements, while at the same time the differential gravitational effects reduce the cluster mass. |
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