Physics
Scientific paper
Sep 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010cxo..prop.3035a&link_type=abstract
Chandra proposal ID #12200943
Physics
Scientific paper
FK Comae is an ultra-fast rotating, single yellow giant, product of a recent W UMa merger. Extraordinary levels of FUV and X-ray emission rate FK Comae a coronal powerhouse on par with the most extreme short-period RS CVn binaries. As a single star, FK Comae has clear advantages as a laboratory for exploring high-energy activity. We will bring to bear Hubble's powerful Cosmic Origins Spectrograph, together with Chandra HETGS and groundbased Zeeman Doppler Imaging, to trace -- over two stellar rotations -- spatial relationships between bright FUV patches, extended X-ray emission zones, and the photospheric dark spots, to inform ideas of coronal structure and heating at the outer limits of magnetospheric activity among the coronal cool stars.
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