XMM-Newton Proposal 02019516

Details XMM-Newton Proposal 02019516 XMM-Newton Proposal 02019516

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..108h&link_type=abstract

XMM-Newton Proposal ID #02019516

Computer Science

Hr 402, Hr 1743, Hr 1907, Hr 2035, Hr 2040, Hr 2429, Hr 3347, Hr 4247, Hr 4763, Hr 5777, Hr 5901, Hr 6299, Hr 6688, Hr 7310, Hr 7429, Hr 8694, Xmm-Newton Proposal 02019516

Scientific paper

We propose to observe 16 nearby late-type giants in order to perform a study of a complete volume-limited sample of single late-type giants within 35 pc. Deep EPIC pn observations will yield detections and X-ray fluxes at solar activity level, which is the minimum yet observed in such stars. Substancial constraints are expected towards our understanding of issues like the evolution of stellar activity in post main-sequence phases, the mechanisms of dynamo action in giant stars, and the scatter of activity in stars of similar properties and evolutionary stage.

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