Other
Scientific paper
Nov 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1273..275t&link_type=abstract
17TH EUROPEAN WHITE DWARF WORKSHOP. AIP Conference Proceedings, Volume 1273, pp. 275-278 (2010).
Other
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.
Ferrario Lilia
Lau Herbert H. B.
Pringle James E.
Tout Christopher A.
Wickramasinghe Dayal T.
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