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We present Herschel dust continuum, James Clerk Maxwell Telescope CO (3–2) observations and a search for [C ii] 158 m and [O i] 63 m spectral line emission for the brightest early‐type dwarf satellite of Andromeda, NGC 205. While direct gas measurements [Mg∼ 1.5 × 106 M⊙, H i+ CO (1–0)] have proven to be inconsistent with theoretical predictions of the current gas reservoir in NGC 205 (>107 M⊙),...
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