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arXiv · astro-ph/0601031

INTEGRAL/RossiXTE high-energy observation of a state transition of GX 339-4

Abstract

On 2004 August 15, we observed a fast (shorter than 10 hours) state transition in the bright black-hole transient GX 339-4 simultaneously with RossiXTE and INTEGRAL. This transition was evident both in timing and spectral properties. Combining the data from PCA, HEXTE and IBIS, we obtained good quality broad-band (3-200 keV) energy spectra before and after the transition. These spectra indicate that the hard component steepened. Also, the high-energy cutoff that was present at ~70 keV before the transition was not detected after the transition. This is the first time that an accurate determination of the broad-band spectrum across such a transition has been measured on a short time scale. It shows that, although some spectral parameters do not change abruptly through the transition, the high-energy cutoff increases/disappears rather fast. These results constitute a benchmark on which to test theoretical models for the production of the hard component in these systems.

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BibTeXRIS

T. Belloni, I. Parolin, M. Del Santo, J. Homan, P. Casella, R. P. Fender, W. H. G. Lewin, M. Mendez, J. M. Miller, M. van der Klis. 2006-01-02. INTEGRAL/RossiXTE high-energy observation of a state transition of GX 339-4. https://doi.org/10.1111/j.1365-2966.2006.09999.x

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