The Coronal Spectra of Post-T Tauri Stars in the Nearby Tucanae Association

Details The Coronal Spectra of Post-T Tauri Stars in the Nearby Tucanae Association The Coronal Spectra of Post-T Tauri Stars in the Nearby Tucanae Association

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1127s&link_type=abstract

Chandra Proposal ID #04200106

Physics

Chandra Proposal Id #04200106

Scientific paper

We propose to observe the two X-ray brightest single young (10-20 Myr) late-type stars of the recently discovered nearby Tucanae Association. The collected HETG spectra will allow the unique opportunity of characterizing the properties of coronae of late-type active single stars still on the radiative track while contracting toward the main-sequence. This will allow us to investigate the effect of binarity versus youth in determinig the shape of differential emission measure distribution and abundances of stellar coronae in a region of the age-activity-rotation parameter space still essentially unexplored.

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