Episodic Accretion onto Neutron Stars and Cosmic Gamma-Ray Bursts

Details Episodic Accretion onto Neutron Stars and Cosmic Gamma-Ray Bursts Episodic Accretion onto Neutron Stars and Cosmic Gamma-Ray Bursts

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pthph..59..425t&link_type=abstract

Progress of Theoretical Physics, Vol. 59, No. 2, pp. 425-434

Physics

2

Scientific paper

The episodic accretion of gas onto the magnetopause of a magnetic neutron star is examined numerically for three different initial distributions and velocities of the accreting gas. The dynamical and thermal structure of the γ-ray emission zone on the magnetopause is determined and the time profile of emergent γ-rays is calculated. The possible relevance of the model calculations and observations of cosmic γ-ray bursts is discussed. In order to reconcile the model calculations with observations, however, it is needed that burst sources are located at distances 10 ˜ 20 pc.

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