Magnetar-driven bubbles and the origin of collimated outflows in gamma-ray bursts
Open Access
- 3 September 2007
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 380 (4) , 1541-1553
- https://doi.org/10.1111/j.1365-2966.2007.12164.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 62 references indexed in Scilit:
- Simulations of Magnetically Driven Supernova and Hypernova Explosions in the Context of Rapid RotationThe Astrophysical Journal, 2007
- Relativistic magnetohydrodynamics winds from rotating neutron starsMonthly Notices of the Royal Astronomical Society, 2006
- Magnetars in the Metagalaxy: An Origin for Ultra–High‐Energy Cosmic Rays in the Nearby UniverseThe Astrophysical Journal, 2003
- Pulsar bow-shock nebulaeAstronomy & Astrophysics, 2002
- The Central X‐Ray Point Source in Cassiopeia AThe Astrophysical Journal, 2001
- Ultra–High-Energy Cosmic Rays from Young Neutron Star WindsThe Astrophysical Journal, 2000
- Exact, Algebraic Solutions of the Thin-Shell Two-Wind Interaction ProblemThe Astrophysical Journal, 1996
- Magnetic shaping of planetary nebulae and other stellar wind bubblesThe Astrophysical Journal, 1994
- An axisymmetric magnetohydrodynamic model for the Crab pulsar wind bubbleThe Astrophysical Journal, 1992
- Speculations on the fizzled collapse of a massive starThe Astrophysical Journal, 1986