Transition of H 1743-322 to the HIMS/SIMS confirmed and preliminary spectral fit results

Details Transition of H 1743-322 to the HIMS/SIMS confirmed and preliminary spectral fit results Transition of H 1743-322 to the HIMS/SIMS confirmed and preliminary spectral fit results

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1813....1c&link_type=abstract

The Astronomer's Telegram, #1813

Astronomy and Astrophysics

Astronomy

1

X-Ray, Gamma Ray, Binaries, Black Holes, Transients, Variables

Scientific paper

We present the results of preliminary spectral fits to the third 130 ksec INTEGRAL ToO observation of H 1743-322 (see ATEL #1779 and ATEL #1798), obtained between 2008-10-23T00:43 and 2008-10-24T14:48. We made joint spectral fits to spectra obtained with the JEM-X (5-20 keV), IBIS/ISGRI (18-200 keV) and SPI (25-200 keV) instruments. The spectrum is no longer described by a purely absorbed thermal Comptonization model of seed photons from the inner disk.

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