Publication
Mon. Not. R. Astron. Soc.
Paper

Hierarchical star formation from the time-space distribution of star clusters in the Large Magellanic Cloud

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Abstract

The average age difference between pairs of star clusters in the Large Magellanic Cloud (LMC) increases with their separation as the ∼0.35 power. This suggests that star formation is hierarchical in space and in time. Small regions form stars quickly and large regions, which often contain the small regions, form stars over a longer period. A similar result found previously for Cepheid variables is statistically less certain than the cluster result.

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Publication

Mon. Not. R. Astron. Soc.

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