The atmospheric heating of AB Dor

Details The atmospheric heating of AB Dor The atmospheric heating of AB Dor

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008xmm..prop...59w&link_type=abstract

XMM-Newton Proposal ID #06022401

Computer Science

Stars, White Dwarfs, Solar System, Ab Dor

Scientific paper

We propose simultaneous XMM-Newton/VLT-UVES observations of the bright ultrafast rotating late-type star AB Dor at X-ray, near UV and optical wavelengths. We intend to study highly time-resolved correlations of coronal, chromospheric and photospheric activity phenomena. AB Dor is a unique target in this context because it permits an unprecedented temporal resolution, comparable to state-of-the-art high-resolution solar spectroscopy. The requirement of strictly simultaneous observations results from the short-lived nature of the activity signatures under study.

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