The EUV Spectrum of Au Mic

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Session 38 -- EUVE -- Astronomy II
Oral presentation, Tuesday, 2:00-6:30, Zellerbach Auditorium Room

[38.09] The EUV Spectrum of Au Mic

B. C. Monsignori Fossi (Osservatoriao Astrofisico di Arcetri), M. Landini (Dipartimento di Astronomia e Sciencza dello Spazio)

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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