The profile of the Fe Kalpha line in the Broad Line Radio Galaxy 3C382

Details The profile of the Fe Kalpha line in the Broad Line Radio Galaxy 3C382 The profile of the Fe Kalpha line in the Broad Line Radio Galaxy 3C382

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cxo..prop.1536s&link_type=abstract

Chandra Proposal ID #05701042

Computer Science

Chandra Proposal Id #05701042

Scientific paper

We propose HETG observations of the X-ray bright Broad-Line Radio Galaxy 3C~382 to study the profile of its strong Fe Kalpha line, and RXTE observations to constrain the broad-band continuum. We have 10 ks of XMM EPIC exposure for this target, soon to be performed. The HETG spectrum will allow us to determine the parameters of the narrow-line component, while the EPIC spectrum will constrain the broad-line component. The proposed observations will allow us to discriminate among competing scenarios for the origin of the Fe line in radio-loud AGN, and determine the structure of the accretion flow in these sources. Chandra is the only instrument with the necessary spectral resolution to resolve the narrow-line component, which in turn is crucial for interpreting the XMM data.

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