Detailed Study of X-ray Jets from a Complete Survey

Details Detailed Study of X-ray Jets from a Complete Survey Detailed Study of X-ray Jets from a Complete Survey

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003hst..prop10002p&link_type=abstract

HST Proposal ID #10002

Physics

Hst Proposal Id #10002 Agn

Scientific paper

We propose deep followup HST and Chandra observations of two X-ray jets, which are the X-ray brightest discovered in our Chandra survey of quasars with known radio jets. With these data, we will compare their X-ray, optical and radio morphologies. We will also obtain X-ray and optical spectral indices, and spatially resolved SEDs from the radio through the X-rays. This will allow us to determine the X-ray emission mechanism at each point in these jets, and test critical predictions made by each mechanism. We will also be able to track any changes in physical conditions {including magnetic field and bulk Lorentz factor} that are present in the observed 90 degree bends.

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