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Di laman Tinggalan supernova:
"Tinggalan supernova dianggap sebagai sumber sinar kosmos galaksi utama.[1][2][3] Hubungan antara sinar kosmos dan supernova pertama kali dicadangkan oleh Walter Baade dan Fritz Zwicky pada tahun 1934. Vitaly Ginzburg dan Sergei Syrovatskii pada tahun 1964 menyatakan bahawa jika kecekapan percepatan sinar kosmos di tinggalan supernova adalah sekitar 10 peratus, sinar kosmos kehilangan Bima Sakti dikompensasi. Hipotesis ini disokong oleh mekanisme tertentu yang dipanggil "pecutan gelombang kejutan" berdasarkan idea Enrico Fermi, yang masih dalam pembangunan.[perlu rujukan]
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