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- W3118124546 abstract "Young stellar groupings and clusters have hierarchical patterns ranging from flocculent spiral arms and star complexes on the largest scale to OB associations, OB subgroups, small loose groups, clusters and cluster subclumps on the smallest scales. There is no obvious transition in morphology at the cluster boundary, suggesting that clusters are only the inner parts of the hierarchy where stars have had enough time to mix. The power-law cluster mass function follows from this hierarchical structure: n(M_cl) M_cl^-b for b~2. This value of b is independently required by the observation that the summed IMFs from many clusters in a galaxy equals approximately the IMF of each cluster." @default.
- W3118124546 created "2021-01-05" @default.
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- W3118124546 date "2006-05-19" @default.
- W3118124546 modified "2023-09-27" @default.
- W3118124546 title "Hierarchical Formation of Galactic Clusters" @default.
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- W3118124546 hasPublicationYear "2006" @default.
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