... G characteristics of particle acceleration by cluster accretion shocks · e n e rg e t i c s 1 0 4 0 e rg /(s M p c 3) a t p re s e n t epoc h, z = 0 SN 3в10 -1 AGN 1 c lu s te r in G R B a c c re t i o n c o s m i c r a y s 3 в 1 0 -2 a t < 1 0 1 5 m aV g ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2007/presentations/25.12.2007/03-ptuskin.pdf -- 562.9 Кб -- 30.01.2008 Похожие документы
... These properties put the quasar 3C 279 into the blazar sub-class of AGN. ... According to the unified model of Active Galactic Nuclei (AGN), blazars are sources which expel jets close to our line-of-sight ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/D35_Collmar01-27Feb07_19:21:51.pdf -- 260.7 Кб -- 27.02.2007 Похожие документы
... 418..844G . Review of GRANAT observations of AGNs. // Multi-Wavelength Continuum Emission of AGN (1994) Churazov, E. M., et al. 1994IAUS..159...63C . ...
... 418..844G . Review of GRANAT observations of AGNs. // Multi-Wavelength Continuum Emission of AGN (1994) Churazov, E. M., et al. 1994IAUS..159...63C . ...
... In R. Mujica and R. Maiolino, editors, Multiwavelength AGN Surveys, page 323. ... 13] E. Boldt. Is AGN Spectral Evolution Needed for the CXB? ... Noordwijk: ESTEC, 1989. 14] E. Boldt. The AGN contribution to the Xray background. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/C04_Frontera01-16Feb07_16:29:39.pdf -- 178.9 Кб -- 16.02.2007 Похожие документы