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

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1841....1b&link_type=abstract

The Astronomer's Telegram, #1841

Astronomy and Astrophysics

Astronomy

1

X-Ray, Binaries, Black Holes, Transients

Scientific paper

We observed the Galactic black hole candidate H 1743-322 on 2008 October 07 for approximately 32 ksec, while the source was in a low/hard state. Here we report the preliminary results of spectral fits to XIS spectra made over the 1.0-10.0 keV band. Spectra from the three XIS detectors were fit jointly using XSPEC. We find that the spectra can be fit with a single power-law, with an index of Gamma = 1.60+/-0.01, with a column density of 2.10 +/- 0.01 E+22.

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