Stellar Coronal Spectroscopy of Cool Stars

Details Stellar Coronal Spectroscopy of Cool Stars Stellar Coronal Spectroscopy of Cool Stars

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cxo..prop..213c&link_type=abstract

Chandra Proposal ID #01200029

Physics

Chandra Proposal Id #01200029

Scientific paper

HETGS spectra will reveal a wealth of information on the temperature and density structure of stellar coronae. In addition, rotational or eclipse modulation can be used to further determine geometric structure. Two RS CVn stars will be observed with HETG and ACIS-S: AR Lac, and II Peg. AR Lac data will be taken through primary eclipse to map emitting structures. One pre-main-sequence star, TW Hya, which is a nearby, isolated, classical T Tauri object, will provide detail on the nature of young-star X-ray emission.

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