The Circumnuclear X-Ray Environments of Highly Disturbed Seyfert Galaxies

Details The Circumnuclear X-Ray Environments of Highly Disturbed Seyfert Galaxies The Circumnuclear X-Ray Environments of Highly Disturbed Seyfert Galaxies

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006cxo..prop.2218e&link_type=abstract

Chandra Proposal ID #08700819

Computer Science

Chandra Proposal Id #08700819

Scientific paper

We propose 60 ks and 35 ks Chandra/ACIS-S observations of the optically disturbed circumnuclear narrow-line environments of the ``radio-loud'' Seyfert 2 galaxies Mrk 573 and IC 5063. We will use Chandra's superb spatial resolution to explore the complex relationship between the X-ray-emitting shock-heated gas, radio outflows, and optical line-emission. We will determine the role of shocks in imparting energy into the ambient ISM, assess the part that ionizing nuclear radiation plays in governing the narrow-line morphology, and constrain the energy budgets involved in creating such disturbed circumnuclear environments.

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