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Australian Journal of Physics
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Australian Journal of Physics
Article . 1992 . Peer-reviewed
License: https://doi.org/10.1071/journalslicense
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Young Star Clusters in the LMC

descriptionPublicationkeyboard_double_arrow_right Article 01 Aug 1992 English Publisher:CSIRO PublishingJournal:Australian Journal of Physics, volume 45, pages 407-410 (issn: 0004-9506, eissn: 1446-5582, Copyright policy )
Authors: KC Freeman;

doi: 10.1071/ph920407

Young Star Clusters in the LMC

Abstract

The young globular star clusters in the LMC offer us insights into the formation and early dynamical evolution of globular clusters which are unobtainable from the old globular clusters in our Galaxy. Because these young clusters are so young and populous, they provide an opportunity to measure the upper end of the initial mass function by direct means and also through the dynamical effects of stellar mass loss on the structure of the clusters.

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selected citations
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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