Searching for nova shells around cataclysmic variables - II. A second campaign

Bibcode
2022MNRAS.510.4180S
DOI
10.1093/mnras/stab3668
Sahman, D. I.; Dhillon, V. S.
Bibliographical reference

Monthly Notices of the Royal Astronomical Society

Advertised on:
3
2022
Journal
Monthly Notices of the Royal Astronomical Society
Number of authors
2
IAC number of authors
1
Citations
4
Refereed citations
3
Description
We report on our second campaign to search for old nova shells around cataclysmic variables (CVs). Our aim was to test the theory that nova eruptions cause cycles in the mass transfer rates of CVs. These mass transfer cycles change the behaviour of CVs during their intereruption periods. We examined Hα images of 47 objects and found no new shells around any of the targets. Combining our latest results with those of our previous campaign (Sahman et al.), and the searches by Schmidtobreick et al. and Pagnotta & Zurek, we estimate that the nova-like phase of the mass transfer cycle lasts ~3000 yr.
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Montserrat
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In progress
Type
Refereed
Stellar & Interstellar Physics (FEEI)
Novae

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