IUE and VIA Observations of the Nearby Dwarf M Flare Stars YY Gem, YZ CMI & AD LEO

Details IUE and VIA Observations of the Nearby Dwarf M Flare Stars YY Gem, YZ CMI & AD LEO IUE and VIA Observations of the Nearby Dwarf M Flare Stars YY Gem, YZ CMI & AD LEO

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iue..prop.1839l&link_type=abstract

IUE Proposal ID #FSGKL

Physics

Scientific paper

We! propose simultaneous ultraviolet and radio wavelength observations of the nearby dwarf M stars YY Gem, YZ Cmi and AD Leo which are known to emit frequent and powerful flares. The combined observations will determine physical conditions such as; electron temperature, electron density and magnetic field strength at a variety, of levels in the stellar atmosphere. They will provide valuable new insights to such things as the difference between coronal and chromospheric flares, the flare energy budget, the flare conditions in the transition region and corona, the magnetic field strength and size of the emitter, the response of the stellar atmosphere to nonthermal events, the location of flare energy release, and preburst heating or magnetic changes that may trigger flare emission.

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