A Time-resolved Extreme-Ultraviolet Spectroscopic Study of the Quiescent and Flaring Corona of the Flare Star AU Microscopii

Details A Time-resolved Extreme-Ultraviolet Spectroscopic Study of the Quiescent and Flaring Corona of the Flare Star AU Microscopii A Time-resolved Extreme-Ultraviolet Spectroscopic Study of the Quiescent and Flaring Corona of the Flare Star AU Microscopii

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...466..427m&link_type=abstract

Astrophysical Journal v.466, p.427

Astronomy and Astrophysics

Astronomy

25

Stars: Coronae, Stars: Flare, Stars: Individual Constellation Name: Au Microscopii, Ultraviolet: Stars

Scientific paper

The extreme-ultraviolet emission measured during a 1992 July 14-17 observation of AU Mic has been studied with lines detected with the short-, medium-, and long-wavelength spectrometers on the Extreme Ultraviolet Explorer. Flares were observed during this period. The time evolution of the differential emission measure is presented. The synthetic spectrum derived from the differential emission measure is compared with the observed data. An estimate of the density and volume of the emitting plasma is obtained by use of Fe XXI lines.

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