Association between Recurrent Novae and Nova Super-Remnants

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Publicado en:arXiv.org (Dec 5, 2024), p. n/a
Autor principal: Healy-Kalesh, Michael William
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Cornell University Library, arXiv.org
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Acceso en línea:Citation/Abstract
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022 |a 2331-8422 
035 |a 3133539295 
045 0 |b d20241205 
100 1 |a Healy-Kalesh, Michael William 
245 1 |a Association between Recurrent Novae and Nova Super-Remnants 
260 |b Cornell University Library, arXiv.org  |c Dec 5, 2024 
513 |a Working Paper 
520 3 |a Nova super-remnants (NSRs) are substantially extended structures (up to ~130 parsecs across) encompassing recurrent novae. NSRs grow as a result of frequent nova eruptions transporting vast quantities of the locally surrounding interstellar medium away from the binary system over many millennia into a thin high-density shell, as the central white dwarf grows towards the Chandrasekhar limit. The prototypical NSR, first identified as such in 2014, is situated in the Andromeda Galaxy and belongs to the annually erupting nova, M31N 2008-12a (or '12a'). In this short review, modelling of evolving NSRs (including the 12a NSR) will be outlined as motivation towards searching for more of these phenomena in the Galaxy and beyond. The latest developments in this upcoming subfield of nova research will then be presented including the discovery of two new Galactic nova super-remnants (and their consequent modelling) and the first survey undertaken with the sole purpose of finding NSRs in the Andromeda Galaxy and the Large Magellanic Cloud. 
653 |a Dwarf galaxies 
653 |a Andromeda Galaxy 
653 |a Novae 
653 |a Dwarf novae 
653 |a Interstellar matter 
653 |a White dwarf stars 
653 |a Magellanic clouds 
653 |a Astronomical models 
773 0 |t arXiv.org  |g (Dec 5, 2024), p. n/a 
786 0 |d ProQuest  |t Engineering Database 
856 4 1 |3 Citation/Abstract  |u https://www.proquest.com/docview/3133539295/abstract/embedded/6A8EOT78XXH2IG52?source=fedsrch 
856 4 0 |3 Full text outside of ProQuest  |u http://arxiv.org/abs/2411.17652