ASKAP monitoring at 887.5 MHz found three classical novae whose steep early radio flares are better matched by a broken-power-law synchrotron model than by thermal free-free emission.
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Radio Monitoring of Classical Novae using the ASKAP Variable and Slow Transients Survey
ASKAP monitoring at 887.5 MHz found three classical novae whose steep early radio flares are better matched by a broken-power-law synchrotron model than by thermal free-free emission.