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首页> 外文期刊>The Astrophysical journal >DETECTION OF A FULLY RESOLVED COMPTON SHOULDER OF THE IRON Kα LINE IN THE CHANDRA X-RAY SPECTRUM OF GX 301-2
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DETECTION OF A FULLY RESOLVED COMPTON SHOULDER OF THE IRON Kα LINE IN THE CHANDRA X-RAY SPECTRUM OF GX 301-2

机译:GX 301-2的钱德拉X射线光谱中铁Kα线的完全分辨康普顿肩峰的检测

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We report the detection of a fully resolved, Compton-scattered emission line in the X-ray spectrum of the massive binary GX 301-2 obtained with the High Energy Transmission Grating Spectrometer on board the Chandra X-Ray Observatory. The iron Kα fluorescence line complex observed in this system consists of an intense narrow component centered at an energy of E = 6.40 keV and a redward shoulder that extends down to ~6.24 keV, which corresponds to an energy shift of a Compton backscattered iron Kα photon. From detailed Monte Carlo simulations and comparisons with the observed spectra, we are able to directly constrain the physical properties of the scattering medium, including the electron temperature and column density, as well as an estimate for the metal abundance.
机译:我们报告了在Chandra X射线天文台上用高能透射光栅光谱仪获得的大规模二元GX 301-2的X射线光谱中检测到的一条完全分解的康普顿散射发射线的检测结果。在该系统中观察到的铁Kα荧光谱线复合物由一个以E = 6.40 keV的能量为中心的强烈狭窄成分和一个向下延伸到〜6.24 keV的红肩峰组成,这对应于康普顿背向散射的Kα铁光子的能量位移。通过详细的蒙特卡洛模拟以及与观察到的光谱的比较,我们能够直接限制散射介质的物理特性,包括电子温度和柱密度,以及金属丰度的估计值。

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