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The Propagation and Eruption of Relativistic Jets from the Stellar Progenitors of Gamma‐Ray Bursts

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Zhang, Weiqun, Woosley, S. E., Heger, A.·2004·The Astrophysical Journal

Abstract

New two- and three-dimensional calculations are presented of relativistic jet propagation and break out in massive Wolf-Rayet stars. Such jets are thought to be responsible for gamma-ray bursts. As it erupts, the highly relativistic jet core (3° to 5°; Γ ≳ 100) is surrounded by a cocoon of less energetic, but still moderately relativistic ejecta (Γ ~ 15) that expands and becomes visible at larger polar angles (~10°). These less energetic ejecta may be the origin of X-ray flashes and other high-energy transients, which will be visible to a larger fraction of the sky, albeit to a shorter distance than common gamma-ray bursts. Jet stability is also examined in three-dimensional calculations. If the jet changes angle by more than 3° in several seconds, it will dissipate, producing a broad beam with inadequate Lorentz factor to make a common gamma-ray burst. This may be an alternate way to make X-ray flashes.

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Metadata

Authors
Zhang, W., Woosley, S. E., & Heger, A.
Venue
The Astrophysical Journal
Published
2004-06-10
Volume
608
Issue
1
Pages
365-377
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2028632015
Cited by
265
References
0
FWCI
15.36
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: The Propagation and Eruption of Relativistic Jets from the Stellar Progenitors of Gamma‐Ray Bursts. https://app.cochat.ai/papers/10.1086/386300
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Zhang, W., Woosley, S. E., & Heger, A. (2004). The Propagation and Eruption of Relativistic Jets from the Stellar Progenitors of Gamma‐Ray Bursts. The Astrophysical Journal. https://doi.org/10.1086/386300

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.