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Discovery of a Transient Absorption Edge in the X-ray Spectrum of GRB 990705

机译:在GRB 990705的X射线光谱中发现瞬态吸收边

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We report the discovery of a transient equivalent hydrogen column density with an absorption edge at ~3.8 kiloelectron volts in the spectrum of the prompt x-ray emission of gamma-ray burst (GRB) 990705. This feature can be satisfactorily modeled with a photoelectric absorption by a medium located at a redshift of ~0.86 and with an iron abundance of ~75 times the solar one. The transient behavior is attributed to the strong ionization produced in the cir-cumburst medium by the GRB photons. The high iron abundance points to the existence of a burst environment enriched by a supernova along the line of sight. The supernova explosion is estimated to have occurred about 10 years before the burst. Our results agree with models in which GRBs originate from the collapse of very massive stars and are preceded by a supernova event.
机译:我们报告了在瞬态等效氢柱密度的发现,在γ射线猝发(GRB)990705的快速X射线发射光谱中,吸收边约为3.8千电子伏。该特征可以通过光电吸收来令人满意地建模。由红移〜0.86的铁和铁丰度约为日照的〜75倍的介质组成。瞬态行为归因于GRB光子在cir-cumburst介质中产生的强电离作用。高铁含量表明存在一个爆炸环境,该环境被沿视线的超新星所丰富。据估计,超新星爆炸发生在爆发前约十年。我们的结果与其中GRB起源于非常大的恒星坍缩并先于超新星事件发生的模型相吻合。

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