XMM-Newton Proposal 03000002

Details XMM-Newton Proposal 03000002 XMM-Newton Proposal 03000002

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop....1s&link_type=abstract

XMM-Newton Proposal ID #03000002

Computer Science

Stars, White Dwarfs, Solar System, Ar Psc, Xmm-Newton Proposal 03000002

Scientific paper

The long-debated issue of the coronal abundances in active stars has not yet arrived to conclusive results, in large part because for most of the stars for which coronal abundances have been determined, no published photospheric abundances are available. This is specially true for the most active stars, in which large rotational velocity complicates the measurement of photospheric abundances. We propose to determine the coronal abundances of a sample of active stars with low projected rotational velocities, for which we have determined accurate photospheric abundances.

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