Multiple Sub-Jet Model of Gamma Ray Bursts and Possible Origin of X-ray Precursors and Post-cursors
arXiv:astro-ph/0004008 · doi:10.1086/312663
Abstract
We assume that internal shocks of Gamma Ray Bursts (GRBs) consist of multiple sub-jets with a collimation half-angle , where is the Lorenz factor of each sub-jet. If by chance a sub-jet is first emitted off-axis from the line of sight, the observed peak energy can be in the X-ray region. Next if by chance a subsequent sub-jet is emitted along the line of sight, then the peak energy will be in the gamma ray region and the gamma ray may arrive after the X-ray precursor from the former sub-jet depending on parameters. This model predicts a new class of GRBs with extremely weak and short gamma ray emission but X-ray precursor and/or post-cursor as well as an afterglow.
6 pages, Latex, accepted for publication in Astrophysical Journal Letters
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- GRB 061121: Broadband spectral evolution through the prompt and afterglow phases of a bright burst
- A Unified Model of Short and Long Gamma-Ray Bursts, X-Ray Rich Gamma-Ray Bursts, and X-Ray Flashes
- Collimated Jet or Expanding Outflow: Possible Origins of GRBs and X-Ray Flashes
- Shallow Decay of Early X-ray Afterglows from Inhomogeneous Gamma-Ray Burst Jets
- Ep-Eiso Correlation in a Multiple Subjet Model of Gamma-Ray Bursts
- The afterglow and complex environment of the optically dim burst GRB 980613
- Tail Emission of Prompt Gamma-Ray Burst Jets
- Short and Long GRBs: same emission mechanism?
- Multi-color Shallow Decay and Chromatic Breaks in the GRB 050319 Optical Afterglow
- Possible Origin of Lognormal Distributions in Gamma-Ray Bursts
- Delayed Flashes from Counter Jets of Gamma Ray Bursts
- Very early multi-color observations of the plateau phase of GRB 041006 afterglow
- A Possible Origin of Bimodal Distribution of Gamma-Ray Bursts
- Probing the Structure of Gamma-Ray Burst Jets with Steep Decay Phase of their Early X-ray Afterglows
- Unveiling the nature of the Einstein Probe transient EP 241021a
- Plasma Pressure Driven Asymmetric Supernovae and Highly Collimated Gamma-Ray Bursts