BHWed_LinfordJ_ClassicalNovae_V1

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Classical novae are excellent laboratories for studying many astrophysical phenomena. They have complex structures due to interacting outflows. They produce shocks where these outflows collide. They have both thermal and non-thermal emission. They evolve over long time scales and remain visible at radio wavelengths for two to three years. The Next Generation Very Large Array (ngVLA) will prov...

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