Far-infrared properties of flare stars and dM stars

Details Far-infrared properties of flare stars and dM stars Far-infrared properties of flare stars and dM stars

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...343..400m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 343, Aug. 1, 1989, p. 400-408.

Astronomy and Astrophysics

Astronomy

26

Far Infrared Radiation, Flare Stars, M Stars, Stellar Spectrophotometry, Infrared Astronomy Satellite, Stellar Coronas, Stellar Luminosity, Stellar Magnitude

Scientific paper

Results are reported from a search of the IRAS data base for flare stars and for a control sample of dM stars. At 12 microns, 70-80 percent of both samples have been detected. The K-12 colors of flare stars are significantly different from those of dM stars: for a given K magnitude, a flare star is about 70 percent brighter at 12 microns than a dM star. At 100 microns, 27 percent of the flare stars which are sources at 12 microns have been detected, while none of the comparable dM stars has been detected. Implications for microflaring are discussed.

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