High-Resolution Spectroscopy of the Classical T Tauri Star SU AUR

Details High-Resolution Spectroscopy of the Classical T Tauri Star SU AUR High-Resolution Spectroscopy of the Classical T Tauri Star SU AUR

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1142s&link_type=abstract

Chandra Proposal ID #04200436

Computer Science

Chandra Proposal Id #04200436

Scientific paper

We propose to obtain high-resolution HETG spectra of the Classical T Tauri star SU Aur. Classical T Tauri stars are unique amongst magnetically active late-type stars, in that they are accreting material from a circumstellar disc. Their magnetospheres therefore contain higher density plasma than a normal M-dwarf or RS CVn. Complex kinematic behaviour is expected from the infalling plasma. Furthermore, the interaction between stellar magnetic field and inner disc may drive reconnection in the magnetosphere. All these processes can be probed in unprecedented detail by Chandra.

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