Alternate: Magnified Views of Quasar Outflows

Details Alternate: Magnified Views of Quasar Outflows Alternate: Magnified Views of Quasar Outflows

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cxo..prop.1733g&link_type=abstract

Chandra Proposal ID #06700036

Physics

Chandra Proposal Id #06700036

Scientific paper

The confirmation of relativistic quasar outflows in most quasars would imply higher mass flow rates than those based on outflow velocities derived from UV BALs. These outflowing winds may thus provide a significant contribution to the enrichment of the vicinity of the quasars and their host galaxies with accretion disk material. To assess the commonality of relativistic outflows in quasars we propose to observed the distant z = 3.6 lensed BALQSO SDSS0903+5028. This is an intriguing object to observe with Chandra because of its relatively high redshift, and cluster lens. We will include SDSS0903+5028 in our sample of high-z lenses radio quiet quasars and verify whether it is consistent with our recently discovered Gamma-LX correlation.

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