A Global Study of X-ray Binaries

R. Dunn, R. Fender, E. Koerding, C. Cabanac, Tomaso Belloni University of Southampton, I. Brera
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引用次数: 1

Abstract

We present preliminary results on a global study of X-ray binaries using 14 Ms of data from the Rossi X-ray Timing Explorer satellite. Our initial study on GX 339-4 is recapped as an introduction to the methods used. We use a consistent analysis scheme for all objects, with three different spectral models to fit the powerlaw and disc components. We also take into account the possibility of a line being present in the data. The resulting almost 4000 observations allow the tracking of the spectral properties of the binaries as they evolve through an outburst. Our investigations concentrate on the disc and line properties of the binaries when in outburst. We also show the Disc-Fraction Luminosity diagram for the population of X-ray binaries studied which will enable us to further links with AGN.
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x射线双星的全球研究
我们提出的初步结果对x射线双星的全球研究使用罗西x射线定时探测器卫星的14ms数据。我们对GX 339-4的初步研究作为所使用方法的介绍进行了重述。我们对所有对象使用一致的分析方案,使用三种不同的光谱模型来拟合幂律和圆盘分量。我们还考虑了数据中存在一条线的可能性。由此产生的近4000次观测可以追踪双星在爆发过程中演变的光谱特性。我们的研究集中在双星突出时的盘状和线状性质。我们还展示了所研究的x射线双星种群的圆盘-分数光度图,这将使我们能够进一步与AGN联系起来。
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