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The Magellanic Edges Survey I: Description, first results · 2007 · DOI 10.1093/mnras/staa2048

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astro-ph.GA 2

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2026 1 2025 1

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Sifting for a Stream: The Morphology of the $300S$ Stellar Stream

astro-ph.GA · 2025-06-26 · unverdicted · novelty 6.0

300S stellar stream exhibits three density peaks, smooth width variations, a possible 4.7 degree gap, and a kink modeled as resulting from Large Magellanic Cloud interaction across its full known footprint.

The VMC survey -- LV. The coherent expansion of the SMC

astro-ph.GA · 2026-06-02 · unverdicted · novelty 4.0

Improved VMC proper motions show SMC expansion along SE-NW axes consistent with LMC tides, radial inward motions with no rotation, and northward motion in older RGB stars from a prior interaction.

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Showing 2 of 2 citing papers after filters.

  • Sifting for a Stream: The Morphology of the $300S$ Stellar Stream astro-ph.GA · 2025-06-26 · unverdicted · none · ref 24

    300S stellar stream exhibits three density peaks, smooth width variations, a possible 4.7 degree gap, and a kink modeled as resulting from Large Magellanic Cloud interaction across its full known footprint.

  • The VMC survey -- LV. The coherent expansion of the SMC astro-ph.GA · 2026-06-02 · unverdicted · none · ref 45

    Improved VMC proper motions show SMC expansion along SE-NW axes consistent with LMC tides, radial inward motions with no rotation, and northward motion in older RGB stars from a prior interaction.