Resolving the Triple Protostar/t Tau System T Tau NS

Details Resolving the Triple Protostar/t Tau System T Tau NS Resolving the Triple Protostar/t Tau System T Tau NS

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1130g&link_type=abstract

Chandra Proposal ID #04200117

Computer Science

Chandra Proposal Id #04200117

Scientific paper

We propose to fully resolve the T Tau N/S system in X-rays for the first time, using the HRC-I on Chandra for 60 ks. The two stars are embedded in envelopes and accrete matter in accretion disks. Several Herbig-Haro objects are present, some of which may produce detectable X-rays as well. A third stellar component has recently been identified; it will be resolved by radio interferometry also proposed. Correlated activity in both wavelength regimes will help associate the emission to particular components and will provide insight into high-energy mechanisms in magnetically accreting protostars.

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