High Energy Gamma Rays from Accretion Disc
作者： F. Giovannelli , S. Karakula , W. Tkaczyk
DOI: 10.1017/S0074180900074842
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摘要: In the case of spherical symmetric accretion into a black hole, matter may be heated up to temperature KT = 0.1 mpc2 (Kolykhalov and Sunyaev, 1979). such hot plasma inelastic collisions protons produce Π° which is gamma quantum source (Dahlbacka et al., 1974; Kolykhalov
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A. W. Strong, A. W. Wolfendale, D. M. Worrall, Origin of the Diffuse - Ray Background Monthly Notices of the Royal Astronomical Society. ,vol. 175, pp. 23P- 27P ,(1976) , 10.1093/MNRAS/175.1.23P
G. H. DAHLBACKA, G. F. CHAPLINE, T. A. WEAVER, Gamma rays from black holes Nature. ,vol. 250, pp. 36- 37 ,(1974) , 10.1038/250036A0
F. Curtis Michel, Accretion of matter by condensed objects Astrophysics and Space Science. ,vol. 15, pp. 153- 160 ,(1972) , 10.1007/BF00649949