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- W1824994968 abstract "The optical radiation of supernova remnants is emitted in density fluctuations or small clouds in which the main shock wave generating thermal x rays is retarded and penetrates the fluctuation from all sides. The gas there has adequate opportunity to cool to optical temperatures. These cloudlets are 5 to 10 times denser than the intervening gas. The shock velocity inside the fluctuations determines the width of the emission lines, while the average Doppler velocity of the filaments depends on the asymmetry of the convergent shock; it is much lower than the main shock velocity." @default.
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- W1824994968 title "Interstellar density fluctuations and the disparity between the optical and X-ray velocities of supernova remnants" @default.
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