High-Resolution Spectroscopy of Active Cool Stars

Details High-Resolution Spectroscopy of Active Cool Stars High-Resolution Spectroscopy of Active Cool Stars

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..436c&link_type=abstract

Chandra Proposal ID #02200047

Physics

Chandra Proposal Id #02200047

Scientific paper

The cool, active binary stars have a forest of coronal emission lines. These prominent features, along with any continuum emission, are diagnostics of the temperature and density structure of coronae, abundances, and geometric extent. Eclipse modulation can provide a direct measurement of coronal geometry. TY Pyx is a 3-day period near-totally eclipsing RS CVn system. We will obtain HETG spectra through the primary eclipse to obtain phase-resolved coronal diagnostics.

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