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The EUV spectra of dMe flare star EQ Pegasi were obtained during a guest observation using the Extreme Ultraviolet Explorer satellite (EUVE) on August 31, 1993. The EQ Peg was detected in all three spectrometer channels, although the LW detection, apart the He II line, was mainly the result of the second order throughput. The main features of the spectra in SW and MW channels are identified: a number of lines are due to highest ionization stages of iron.
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