Preliminary Reults from a Chandra HETG Observation of NGC 3516

Details Preliminary Reults from a Chandra HETG Observation of NGC 3516 Preliminary Reults from a Chandra HETG Observation of NGC 3516

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001tysc.confe..58t&link_type=abstract

Two Years of Science with Chandra, Abstracts from the Symposium held in Washington, DC, 5-7 September, 2001, meeting abstract.

Physics

Active Galaxies And Quasars

Scientific paper

ASCA data showed NGC 3516 to have a broad and redshifted Fe Kα line with an absorption feature at 5.8 keV. We took an HETG observation to confirm the presence of the 5.8 keV feature. The absorption feature is important as it could imply a high velocity infall of some material, this is rarely observed in AGN. The HETG data will also be used to make a detailed study of the ionized gas around the nucleus of this AGN.

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