Coronal and Chromospheric Heating in Active Dwarf Stars

Details Coronal and Chromospheric Heating in Active Dwarf Stars Coronal and Chromospheric Heating in Active Dwarf Stars

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop.3562g&link_type=abstract

Spitzer Proposal ID #3562

Physics

Scientific paper

We propose to observe a sample of highly active M dwarfs with IRAC and MIPS. Such active dwarfs are known to have large infrared excesses. We argue that the excesses are likely to result from the hot chromospheres and coronae above the photosphere. In this context, our proposed measurements of the (excess) infrared spectral energy distribution will allow us to reliably map the temperature rise in the chromosphere.

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