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The Source of Ionization along the Magellanic Stream

ASTROPHYSICAL JOURNAL, no. 2 (2007): L109-L112

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Since its discovery in 1996, the source of the bright H alpha emission (up to 750 mR) along the Magellanic Stream has remained a mystery. There is no evidence of ionizing stars within the H I stream, and the extended hot halo is far too tenuous to drive strong shocks into the clouds. We now present a hydrodynamical model that explains the...更多

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