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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 2 Pith papers

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

  1. LMC-induced Perturbations in the Milky Way Halo:I. HaloDance Simulation Suite and Observational Forecasts

    astro-ph.GA 2025-07 conditional novelty 6.0 of 10

    A 2,848-simulation suite with neural-network emulation forecasts that halo star kinematics can measure Milky Way and LMC masses to about 11% and 16% precision using current survey capabilities.

  2. UVIT Study of the Magellanic Clouds (U-SMAC). III. Hierarchical Star Formation in the Small Magellanic Cloud Regulated by Turbulence

    astro-ph.GA 2025-06 conditional novelty 4.0 of 10

    Young stars in the Small Magellanic Cloud form a fractal-like hierarchy with dimension 1.3 to 1.6, matching the turbulent gas, supporting turbulence-regulated star formation.

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