Moscow 2006 Astro Space Center P.N. Lebedev Physical Institute DCR-1000 - cross 1000х1000 m, width 40 m, range 30-120 MHz. BSA – array of 16384 dipoles,187х384 m, 16…

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Moscow 2006 Astro Space Center P.N. Lebedev Physical Institute DCR-1000 - cross 1000х1000 m, width 40 m, range 30-120 MHz. BSA – array of 16384 dipoles,187х384 m, 16…

Facts about SNe and their remnants Evolution of an SNR sensitively depends on its environment. Observed SNRs are typically produced by SNe in relative dense environments.…

Yu. D. Kotov and CORONAS-PHOTON team Scientific objectives and observational capabilities of "Coronas-Photon" project Federal Space Agency Russian Academy of Science…

Facts about SNe and their remnants Evolution of an SNR sensitively depends on its environment. Observed SNRs are typically produced by SNe in relative dense environments.…

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