The issue of coronal abundances: observation of two active stars with well determined photospheric abundances

Details The issue of coronal abundances: observation of two active stars with well determined photospheric abundances The issue of coronal abundances: observation of two active stars with well determined photospheric abundances

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cxo..prop.1638s&link_type=abstract

Chandra Proposal ID #06200164

Computer Science

Chandra Proposal Id #06200164

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 two active stars with low projected rotational velocities, for which we have determined accurate photospheric abundances.

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