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EXOSAT and IUE observations of the active star Au Mic are used to develop a model of the differential emission measure distribution versus temperature. The signals detectable by the Extreme Ultraviolet Explorer (EUVE) spectrometers are predicted. The computation indicates the presence of several high, ionized iron lines in the EUV spectral region. Comparison is made with incoming observations by Short (70--190~\AA) and Medium (140--380~\AA) wavelengths spectrometers on EUVE.
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