Theoretical Models of a Flare on AU MIC seen by EUVE Deep Survey Detectors

Details Theoretical Models of a Flare on AU MIC seen by EUVE Deep Survey Detectors Theoretical Models of a Flare on AU MIC seen by EUVE Deep Survey Detectors

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...182.4608f&link_type=abstract

American Astronomical Society, 182nd AAS Meeting, #46.08; Bulletin of the American Astronomical Society, Vol. 25, p.875

Astronomy and Astrophysics

Astronomy

Scientific paper

The M-dwarf star AU Mic was observed by the EUVE Deep Survey Instrument from 1992 July 14-18. A large flare with a total radiated energy in the EUV of approximately 3 times 10(34) \ erg was detected in the Lexan/Boron (65-190 Angstroms) band at 12:38 UT on 15 July 1992. These observations are described further in a recent paper (Cully, Siegmund, Vedder and Vallerga Ap. J. Lett, 1993, in press). We present an analysis of this data in terms of theoretical models of flaring loops.

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