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- W201630091 abstract "The spectrum of Cet in the region 80 -370 A observed by EUVE Spectrometers is analyzed to investigate the transition region and the corona of the star. The star appears to be in a rather quiet condition and no evidence exists of flare- like lines observed in many active stars. Several emission lines of moderately ionized iron (from Fe IX to Fe XVIII) are identi- ed and used together with I.U.E. observations to evaluate the differential emission measure (DEM).TheDEMpeaksat about 3 10 6 K , a value typical of solar active regions. This is conrmed by a comparison with the spectrum of an Active Re- gion of the Solar Corona measured by the Coronal Diagnostic Spectrometer on SOHO showing very similar features." @default.
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- W201630091 date "1997-08-20" @default.
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- W201630091 title "The EUV spectrum of κ Ceti: An active Sun" @default.
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