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Supersoft X-ray rebrightening of Nova Mon 2012
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Supersoft X-ray rebrightening of Nova Mon 2012

K. L. Li and A. K. H. Kong
The Astronomer's Telegram
2012

Abstract

X-ray
We report ten consecutive Swift follow-up observations of Nova Mon 2012 (ATel #4590). The first six observations were performed daily from 2012 November 23 to 2012 November 28 (~2 ks exposure per day) and the last four observations (~1 ks each) were taken on 2012 November 29. All Swift/XRT data are in the Photon Counting (PC) mode.

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