Journal Article

Probing the nature of high-<i>z</i> short GRB 090426 with its early optical and X-ray afterglows

Li-Ping Xin, En-Wei Liang, Jian-Yan Wei, Bing Zhang, Hou-Jun Lv, Wei-Kang Zheng, Yuji Urata, Myungshin Im, Jing Wang, Yu-Lei Qiu, Jin-Song Deng, Kui-Yun Huang, Jing-Yao Hu, Yiseul Jeon, Hua-Li Li and Xu-Hui Han

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 410, issue 1, pages 27-32
Published in print January 2011 | ISSN: 0035-8711
Published online December 2010 | e-ISSN: 1365-2966 | DOI: http://dx.doi.org/10.1111/j.1365-2966.2010.17419.x
Probing the nature of high-z short GRB 090426 with its early optical and X-ray afterglows

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GRB 090426 is a short-duration burst detected by Swift ( s in the observer frame and s in the burst frame at z= 2.609). Its host galaxy properties and some gamma-ray-related correlations are analogous to those seen in long-duration gamma-ray bursts (GRBs), which are believed to be of a massive star origin (so-called Type II GRBs). We present the results of its early optical observations with the 0.8-m Tsinghua University–National Astronomical Observatory of China Telescope (TNT) at Xinglong Observatory and the 1-m LOAO telescope at Mt Lemmon Optical Astronomy Observatory in Arizona. Our well-sampled optical afterglow light curve covers from to 104 s after the GRB trigger. It shows two shallow decay episodes that are likely due to energy injection, which end at and 7100 s, respectively. The decay slopes after the injection phases are consistent with each other (). The X-ray afterglow light curve appears to trace the optical, although the second energy-injection phase was missed due to visibility constraints introduced by the Swift orbit. The X-ray spectral index is without temporal evolution. Its decay slope is consistent with the prediction of the forward shock model. Both X-ray and optical emission are consistent with being in the same spectral regime above the cooling frequency (). The fact that is below the optical band from the very early epoch of the observation provides a constraint on the burst environment, which is similar to that seen in classical long-duration GRBs. We therefore suggest that death of a massive star is the possible progenitor of this short burst.

Keywords: gamma-ray burst: individual: GRB 090426; gamma-rays: general

Journal Article.  4124 words.  Illustrated.

Subjects: Astronomy and Astrophysics

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