MUTI-WAVELENGTH OBSERVATIONS of GRB 111228A and IMPLICATIONS for the FIREBALL and ITS ENVIRONMENT

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题名:	MUTI-WAVELENGTH OBSERVATIONS of GRB 111228A and IMPLICATIONS for the FIREBALL and ITS ENVIRONMENT
作者:	浦田裕次;Xin, Li-Ping;Wang, Yuan-Zhu;Lin, Ting-Ting;Liang, En-Wei;Lü, Hou-Jun;Zhong, Shu-Qing;Urata, Yuji;Zhao, Xiao-Hong;Wu, Chao;Wei, Jian-Yan;Huang, Kui-Yun;Qiu, Yu-Lei;Deng, Jin-Song
贡献者:	理學院天文研究所
关键词:	AFTERGLOW;Afterglows;ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;COSMIC DUST;COSMIC GAMMA BURSTS;DENSITY;Engines;Fireballs;GAMMA RADIATION;Gamma ray bursts;Gamma rays;gamma-ray burst: individual (GRB 130702A, GRB 111228A);KEV RANGE 10-100;Lorentz factor;LUMINOSITY;MARKOV PROCESS;MONTE CARLO METHOD;Monte Carlo methods;NEUTRON STARS;X-rays
日期:	2016-02-01
上传时间:	2026-04-21 14:47:55 (UTC+8)
出版者:	IOP Publishing Ltd.;United Kingdom: The American Astronomical Society
摘要:	摘要： ABSTRACT Observations of very early multi-wavelength afterglows are critical to reveal the properties of the radiating fireball and its environment as well as the central engine of gamma-ray bursts (GRBs). We report our optical observations of GRB 111228A from 95 s to about 50 hr after the burst trigger and investigate its properties of the prompt gamma-rays and the ambient medium using our data and the data from the Swift and Fermi missions. Our joint optical and X-ray spectral fits to the afterglow data show that the ambient medium features a low dust-to-gas ratio. Incorporating the energy injection effect, our best fit to the afterglow light curves with the standard afterglow model via the Markov Chain Monte Carlo technique shows that , , cm−3. The low medium density likely implies that the afterglow jet may be in a halo or in a hot ISM. A chromatic shallow decay segment observed in the optical and X-ray bands is well explained with the long-lasting energy injection from the central engine, which would be a magnetar with a period of about 1.92 ms inferred from the data. The Ep of its time-integrated prompt gamma-ray spectrum is ∼26 KeV. Using the initial Lorentz factor ( ) derived from our afterglow model fit, it is found that GRB 111228A satisfies the relation and bridges the typical GRBs and low luminosity GRBs in this relation. 其他題名： APJ 其他題名： Astrophys. J 出版者： United Kingdom: The American Astronomical Society 出版日期： 2016-02-01 出處： The Astrophysical journal, 2016-02, Vol.817 (2), p.152 資源來源： Institute of Physics Journals 版權： 2016. The American Astronomical Society. All rights reserved. 識別號： ISSN: 0004-637X 識別號： ISSN: 1538-4357 識別號： EISSN: 1538-4357 識別號： DOI: 10.3847/0004-637X/817/2/152
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