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OSCIR Unveils Rich Dust Content in the Second Most Metal Deficient Galaxy Known

The infrared spectral energy distribution of the emitting dust in SBS 0334-52.

The infrared spectral energy distribution of the emitting dust in SBS 0334-52.

For more information, see: http://www.gemini.edu/science/oscir.html


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Gemini Observatory
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Gemini Observatory
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Last updated by Virginia Smith / web@gemini.edu / October 9, 2002