A Study of the Physics of Extended Relativistic X-ray Jets, Discovered in our Chandra Survey

Details A Study of the Physics of Extended Relativistic X-ray Jets, Discovered in our Chandra Survey A Study of the Physics of Extended Relativistic X-ray Jets, Discovered in our Chandra Survey

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cxo..prop.1762g&link_type=abstract

Chandra Proposal ID #06700990

Physics

Chandra Proposal Id #06700990

Scientific paper

We will measure the changing flow speeds, magnetic fields, and energy fluxes in six well-resolved quasar jets found in our short-exposure Chandra survey by combining new, deep Chandra data with radio and optical imaging. We will image each jet with sufficient sensitivity to estimate beaming factors and magnetic fields in several distinct regions, and so map the variations in these parameters down the jets. HST observations will help diagnose the role of synchrotron emission in the overall SED, and may reveal condensations on scales less than 0.1 arcsec.

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