Physics
Scientific paper
Oct 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop...21w&link_type=abstract
XMM-Newton Proposal ID #04004601
Physics
Stars, White Dwarfs, Solar System, Hd 197890, Xmm-Newton Proposal 04004601
Scientific paper
We propose simultaneous observations of the ultrafast rotating late-type star Speedy Mic at X-ray, near UV and optical wavelengths. In this way we want to study the spatial correlation of coronal, chromospheric and photospheric activity phenomena. The proposed study includes time-resolved high resolution spectroscopy monitoring of key line ratios, probing the distribution of coronal temperatures, densities and elemental abundances.The requirement of strictly simultaneous observations results from the short-lived nature of active regions on Speedy Mic. Our proposal is based on our previous results from VLT measurements constructing a Doppler image of Speedy Mic and finding pronounced rotational modulation of CaII emission.
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