Magellanic Stream

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Galaxies, Individual Galaxies

Scientific paper

The Magellanic Stream (MS), which covers an arc of more than 90° across the sky, is a thin band of neutral hydrogen (H I). It is basically continuous, although there are at least six separate regions within the stream where the particle density is visibly enhanced. One end of the MS appears to be connected with the LARGE and SMALL MAGELLANIC CLOUDS, with the other end trailing away from them (...

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