Accretion induced collapse of white dwarfs and the origin of Long Gamma-Ray Bursts

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Gamma-Ray Sources (Astronomical), Jets, Neutron Stars, White Dwarfs, Magnetic Fields, Gamma-Ray, Jets, Outflows, And Bipolar Flows, Neutron Stars, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Gravitational Radiation, Magnetic Fields, And Other Observations

Scientific paper

The stellar origin of gamma-ray bursts can be explained by the rapid release of energy in a highly collimated, extremely relativistic jet. This in turn appears to require a rapidly spinning highly magnetised stellar core that collapses into a magnetic neutron star or a black hole within a relatively massive envelope. We hypothesize a binary star model that ends with the merging of an oxygen neon white dwarf with the carbon-oxygen core of a naked helium star during a common envelope phase of evolution, and subsequent accretion induced collapse into a neutron star. The rapid spin and high magnetic field are natural consequences of such a merging. These progenitors, being of intermediate mass, differ radically from the usually postulated high-mass stars. Thus we can reconcile observations that the bursts occur close to but not within massive star associations.

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