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The morphology of the Magellanic Clouds revealed by stars of different age: results from the DENIS survey

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arxiv astro-ph/0005057 v1 pith:NOCCXBET submitted 2000-05-03 astro-ph

Maria-Rosa L. Cioni , Harm J. Habing , Frank P. Israel This is my paper · ORCID
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The spatial distribution of sources populating different regions of the colour-magnitude diagram (I-J, I) extracted from the DENIS catalogue towards the Magellanic Clouds (DCMC -- Cioni et al. 2000) reveal significantly different morphologies. Each region is associated to a different age group. The Large Magellanic Cloud (LMC) shows an extended circular shape with a prominent, off center bar, a nucleus and irregular spiral arms. The Small Magellanic Cloud shows a perturbated structure with a prominent central concentration of stars. Old and young populations are offset from one another.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

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