A 3D simulation of nine repeated nova eruptions shows that nested shell collisions produce a slowly fading soft X-ray component and episodic hard X-ray flares, roughly matching the extended X-rays seen around RS Ophiuchi.
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X-rays from shock-heated gas in recurrent-nova remnants: Nested nova shells in a structured circumstellar medium
A 3D simulation of nine repeated nova eruptions shows that nested shell collisions produce a slowly fading soft X-ray component and episodic hard X-ray flares, roughly matching the extended X-rays seen around RS Ophiuchi.