Searching for nova shells around cataclysmic variables
D. I. Sahman, V. S. Dhillon, C. Knigge, T. R. Marsh

TL;DR
This study searched for nova shells around 101 cataclysmic variables using Halpha imaging, discovering one shell around V1315 Aql and evidence of past eruptions in V2275 Cyg, providing insights into nova recurrence and CV evolution.
Contribution
First systematic search for nova shells around a large sample of CVs, identifying new shells and evidence of historical eruptions, enhancing understanding of nova recurrence and CV phases.
Findings
Discovered a nova shell around V1315 Aql, indicating a recent eruption.
Found tentative shell evidence around V1363 Cyg, a dwarf nova.
Detected a light echo around V2275 Cyg, suggesting an earlier eruption.
Abstract
We present the results of a search for nova shells around 101 cataclysmic variables (CVs), using Halpha images taken with the 4.2-m William Herschel Telescope (WHT) and the 2.5-m Isaac Newton Telescope Photometric Halpha Survey of the Northern Galactic Plane (IPHAS). Both telescopes are located on La Palma. We concentrated our WHT search on nova-like variables, whilst our IPHAS search covered all CVs in the IPHAS footprint. We found one shell out of the 24 nova-like variables we examined. The newly discovered shell is around V1315 Aql and has a radius of approx.2.5 arcmin, indicative of a nova eruption approximately 120 years ago. This result is consistent with the idea that the high mass-transfer rate exhibited by nova-like variables is due to enhanced irradiation of the secondary by the hot white dwarf following a recent nova eruption. The implications of our observations for the…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Astronomical Observations and Instrumentation · Astronomy and Astrophysical Research
