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A Recurrent Nova Super-Remnant in the Andromeda Galaxy

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arxiv 1712.04872 v1 pith:2OZBJZTP submitted 2017-12-13 astro-ph.SR astro-ph.HE

M. J. Darnley , R. Hounsell , T. J. O'Brien , P. Rodríguez-Gil , A. W. Shafter , M. M. Shara , M. Henze , M. F. Bode
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R. Galera-Rosillo D. J. Harman J.-U. Ness V. A. R. M. Ribeiro N. M. H. Vaytet S. C. Williams
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keywords novam31nsuper-remnantandromedaannuallydemonstrateseruptederupts
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Here we report that the most rapidly recurring nova, M31N 2008-12a, which erupts annually, is surrounded by a "nova super-remnant" which demonstrates that M31N 2008-12a has erupted with high frequency for millions of years.

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Cited by 1 Pith paper

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  1. Association between Recurrent Novae and Nova Super-Remnants

    astro-ph.GA 2024-11 conditional novelty 2.0 of 10

    A review of nova super-remnants: the prototypical M31N 2008-12a remnant, new Galactic examples around KT Eridani and RS Ophiuchi, and a survey finding none in M31 or the LMC.

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