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Published online by Cambridge University Press: 12 April 2016
We present results from the analysis of spectra of the fast rotating active giant star FK Comae Berenices. The extended emission is interpreted as arising in giant active loops and prominences. The absorption is due to a shell of cold and dense gas (like solar filaments).
Centro de Astrofísica da Universidade do Porto, Portugal
Institut d’Astrophysique Spatial, CNRS, France
Based on Observations with the ESA-MUSICOS spectrograph at the Isaac Newton Telescope, ING Observatory, La Palma, Spain