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Cited article:

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The Magnetohydrodynamics of Shock‐Cloud Interaction in Three Dimensions

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Physical and Chemical Inhomogeneities Inside the Vela SNR Shell: Indications of Ejecta Shrapnels

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The Importance of Magnetic‐Field‐Oriented Thermal Conduction in the Interaction of SNR Shocks with Interstellar Clouds

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