X-ray properties of compact CSS quasar with BALs - 1045+352

Details X-ray properties of compact CSS quasar with BALs - 1045+352 X-ray properties of compact CSS quasar with BALs - 1045+352

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cxo..prop.2440k&link_type=abstract

Chandra Proposal ID #09700792

Computer Science

Chandra Proposal Id #09700792

Scientific paper

We propose a 5 ksec observation with Chandra ACIS-S to detect for the first time an X-ray emission from the high ionization broad absorption line (HiBAL) compact steep spectrum (CSS) radio-loud quasar 1045+352. The X-ray information is critical to studies of the environment of BALQSOs. Radio-loud BALs have important additional information about their orientation based on the radio morphology, but they are rare. Only a handful of radio-loud BALs observed in X-rays so far indicating their high intrinsic absorption columns. The proposed target has a deep radio data and known optical spectrum. The new X-ray Chandra data will put a stringent limit on the absorption column by direct measure of the absorption in the spectrum or suppression of the predicted X-ray flux.

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