State Transition and Flaring Activity of IGR J17464–3213/H1743–322 with INTEGRAL SPI

• Published in: The Astrophysical journal Vol. 629; no. 2; pp. 1008 - 1016
• Main Authors: Joinet, A, Jourdain, E, Malzac, J, Roques, J. P, Schönfelder, V, Ubertini, P, Capitanio, F
• Format: Journal Article
• Language: English
• Published: IOP Publishing 20-08-2005
• ISSN: 0004-637X; 1538-4357
• DOI: 10.1086/431576

IGR J17464-3213, already known as the HEAO 1 transient source H1743-322, has been detected during a state transition by INTEGRAL SPI. We describe the spectral evolution and flaring activity of IGR J17464-3213/H1743-322 from 2003 March 21 to 2003 April 22. During the first part, the source followed a continuous spectral softening, with the peak of the spectral energy distribution shifting from 100 keV down to 6a few keV. However, the thermal disk and the hard X-ray components had a similar intensity, indicating that the source was in an intermediate state throughout our observations and evolving toward the soft state. In the second part of our observations, the RXTE ASM and INTEGRAL SPI light curves showed a strong flaring activity. Two flare events lasting about 1 day each have been detected with SPI and are probably due to instabilities in the accretion disk associated with the state transition. During these flares, the low (1.5-12 keV) and high (20-200 keV) energy fluxes monitored with the RXTE ASM and INTEGRAL SPI are correlated, and the spectral shape (above 20 keV) remains unchanged while the luminosity increases by a factor greater than 2.