Suzaku Observations of H 1743-322: Implications for Disk Winds

Details Suzaku Observations of H 1743-322: Implications for Disk Winds Suzaku Observations of H 1743-322: Implications for Disk Winds

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cfdd.confe..69b&link_type=abstract

Chandra's First Decade of Discovery, Proceedings of the conference held 22-25 September, 2009 in Boston, MA. Edited by Scott Wo

Physics

Accretion And Outflows

Scientific paper

Disk winds can be key to understanding disk physics and inflow-outflow connections in accreting black holes. We observed the black hole candidate H 1743-322 in the low/hard state during the 2008 outburst with Suzaku. The spectra rule-out Fe XXV and Fe XXVI absorption lines, and thus rule-out an ionized disk wind like that previously detected in a disk-dominated high/soft state with Chandra. Our results suggest that the wind is quenched, rather than merely too highly ionized to be detected. This adds to a growing picture that winds and jets are anti-correlated and state-dependent. We will report and discuss our Suzaku results in the context of inflow-outflow connections in accreting systems.

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