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Multiple emission of intermediate-mass fragments has been studied for the collisions of p, He and C on Au with the setup FASA. In the case of C(22.4 GeV)+Au and He(14.6 GeV)+Au collisions, the deviations from a pure thermal break-up are seen in the energy spectra of the emitted fragments: the spectra are harder than calculated and than measured in p-induced collisions. This difference is attributed to a collective flow with the expansion velocity on the surface about 0.1 (for C+Au collisions).

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