DG Tauri: A T Tauri Star with an X-Ray Jet?

Details DG Tauri: A T Tauri Star with an X-Ray Jet? DG Tauri: A T Tauri Star with an X-Ray Jet?

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cxo..prop.1884g&link_type=abstract

Chandra Proposal ID #07200268

Computer Science

Chandra Proposal Id #07200268

Scientific paper

The classical T Tauri star DG Tau A drives one of the nearest and strongest optical jets with protostar-like properties. Recent Chandra observations reveal unusual X-ray properties that may be related to shock emission at the jet base. We propose new, deeper observations to i) image faint emission of jet-shocks out to several arcseconds, ii) to derive the spectral characteristics of this emission, and iii) to compare its spectrum with an unusually soft component in the spectrum of the star itself. We will also obtain a better spectrum of the deeply absorbed protostar DG Tau B as well as of the multiple system FV Tau.

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