Rupen_Radio Imaging of Galactic Explosions

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I explore the use of a next-generation radio interferometer for imaging accretion-powered outbursts in our Galaxy. An array with resolution of order milliarcseconds and the sensitivity to image thermal (<1e4 K) sources would have an enormous impact. I illustrate the possibilities with examples of both thermal (novae) and non-thermal (X-ray binaries) transients, with source ages ranging from days to decades.

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