A mechanism of high-energy-particle generation and corona formation in binary X-ray sources

Details A mechanism of high-energy-particle generation and corona formation in binary X-ray sources A mechanism of high-energy-particle generation and corona formation in binary X-ray sources

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..918g&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, Oct. 1989, p. 918-924. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Accretion Disks, Energetic Particles, Stellar Coronas, X Ray Binaries, Companion Stars, Electric Fields, Gamma Ray Astronomy, Neutron Stars, Particle Acceleration

Scientific paper

A mechanism of electrostatic proton acceleration by electric fields generated by a differentially rotating disk is considered. From a magnetized accretion disk in the case of binary X-ray sources a proton outflow perpendicular to the plane of symmetry of the disk is shown to occur with energies of about 1 TeV and intensity up to about 10 to the 36th erg/s. It is suggested that this mechanism may be important for formation of coronas around binary X-ray sources.

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