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Both the temperature dependence of n0(T) and of the width of n\\star(k) are determined. The n0(T) can be represented by n0(T) = n0(0)[1-(T/T{\\lambda}){\\gamma}] with a small n0(0) = 2.80\\pm0.20% and large {\\gamma} = 13\\pm2 for T < T{\\lambda} indicating strong interaction. The onset of BEC is accompanied by a significant narrowing of the n\\star(k). 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