Decrease in flux of H 1743-322 and preliminary spectral fit results

Details Decrease in flux of H 1743-322 and preliminary spectral fit results Decrease in flux of H 1743-322 and preliminary spectral fit results

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1798....1c&link_type=abstract

The Astronomer's Telegram, #1798

Astronomy and Astrophysics

Astronomy

3

X-Ray, Gamma Ray, Agn, Binaries, Black Holes, Gamma-Ray Bursts, Neutron Stars, Novae, Pulsars, Quasars, Soft Gamma-Ray Repeaters, Transients, Variables, Stars

Scientific paper

We present the results of preliminary spectral fits to the second 130
ksec INTEGRAL ToO observation of H 1743-322 (see ATEL #1779), obtained
between 2008-10-17T20:59 and 2008-10-19T10:17. We made joint spectral
fits to spectra obtained with the JEM-X (5-20 keV), IBIS/ISGRI (18-200
keV) and SPI (23-200 keV) instruments.

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