© Eugene A. Grigor'ev
The possible mechanism of hard radiation
in systems of binary stars
at presence the interstars accretion channel.
As is marked in article "Equations of Maxwell", there is a magnetic field (MF) between two corpuscles, which move to one party (Fig.8). To be convinced of it, it is enough to calculate intensity of MF in points of a matrix shown in a Fig. 1.
Fig. 1
The magnetic intensity of a mobile charged corpuscle can be calculated by formula:
The corpuscles in an accretion channel have longitudinal component of motion in basic. Because of rotation of a system of a binary star (Fig. 2), there is, also, a mutual relative motion of corpuscles of interstellar plasma and an accretion channel (Fig. 3). The cross-sectional (I apologize, but, while, in Russian) oscillations of charged particles occur in a channel. The undulatory radiation with a different wavelength and intensity is generated. (�Maxwell's equations" Fig. 11, �Free Electrones Laser�). The radiation is spread in some cone, and the center of a cone of radiation is screened by a star - acceptor. At rotation of such system the double impulses of radiation (Fig. 2) will be watched.
Fig. 2
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