Dust Scattering Model for X-Ray Afterglows of Gamma-Ray Bursts
Here we report on our recent work on dust scattering in the field of Gamma-Ray Bursts (GRBs), and address that the features of some X-ray afterglows from minutes to days are consistent with the scattering of prompt X-ray emission from GRBs off host dust grains. We propose that some of the observed X-ray afterglows (especially those without sharp rising and decaying flares) could be understood with a dust-scattering- driven emission model.
dust extinction-gamma rays bursts-interstellar medium-X-rays general
L. Shao Z. G. Dai
Department of Astronomy, Nanjing University, Nanjing 210093, China
国际会议
紧凑型物体的天体物理学国际会议(International Conference on Astrophysics of Compact Objects)
安徽黄山
英文
43-45
2007-07-01(万方平台首次上网日期,不代表论文的发表时间)