Star clusters are groups of stars which are gravitationally bound.
Two distinct types of star cluster can be distinguished: globular clusters are tight groups of hundreds of thousands of very old stars, while open clusters generally contain less than a few hundred members, and are often very young.
For more information about the topic Star cluster, read the full article at Wikipedia.org, or see the following related articles:
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Note: This page refers to an article that is licensed under the GNU Free Documentation License. It uses material from the article Star cluster at Wikipedia.org. See the Wikipedia copyright page for more details.
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