Evolution of Magnetic Activity and the Accretion History in Taurus-Auriga Multiple Systems

Details Evolution of Magnetic Activity and the Accretion History in Taurus-Auriga Multiple Systems Evolution of Magnetic Activity and the Accretion History in Taurus-Auriga Multiple Systems

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006cxo..prop.2099g&link_type=abstract

Chandra Proposal ID #08200206

Computer Science

Chandra Proposal Id #08200206

Scientific paper

We request Chandra observing time to survey pre-main sequence binary and multiple systems in the Taurus-Auriga Molecular Cloud (TMC) that can be studied exclusively by Chandra. These systems show separations between components in the range of ~1-5". TMC contains an anomalously high fraction of binaries and is therefore a testbed for binary formation theories. X-ray studies provide important diagnostics related to accretion processes and evolution of the TMC sample. This Chandra project will be an integral part of a large, deep survey of the TMC that has been conducted with the Spitzer Space Telescope, XMM-Newton, and optical and near-infrared ground-based telescopes.

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