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

被引:84
作者
Belloni, T
Parolin, I
Del Santo, M
Homan, J
Casella, P
Fender, RP
Lewin, WHG
Méndez, M
Miller, JM
van der Klis, M
机构
[1] INAF, Osservatorio Astron Brera, I-23807 Merate, Italy
[2] INAF, Ist Astrofis Spaziale & Fis Cosm Roma, I-00133 Rome, Italy
[3] MIT, Ctr Space Res, Cambridge, MA 02139 USA
[4] Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, Hants, England
[5] SRON, Netherlands Inst Space Res, NL-3584 CA Utrecht, Netherlands
[6] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands
[7] Univ Amsterdam, Ctr High Energy Astrophys, NL-1098 SJ Amsterdam, Netherlands
基金
英国科学技术设施理事会;
关键词
accretion; accretion discs; black hole physics; X-rays : binaries;
D O I
10.1111/j.1365-2966.2006.09999.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
On 2004 August 15, we observed a fast (shorter than 10 h) state transition in the bright black hole transient GX 339-4 simultaneously with Rossi X-Ray Timing Explorer (RXTE) and INTEGRAL. This transition was evident both in timing and spectral properties. Combining the data from the Proportional Counter Array (PCA), the High-Energy X-ray Timing Experiment (HEXTE) and the Imager on Board the INTEGRAL Satellite (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 cut-off that was present at similar to 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 cut-off 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.
引用
收藏
页码:1113 / 1120
页数:8
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