Aneurin Evans - A WISE view of novae - I. The data.pdf
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A WISE view of novae - I. The data
Abstract
We present the results of data-mining the Wide-field Infrared Survey Explorer (WISE) archive for data on classical and recurrent novae. We find that the detections are consistent with dust emission, line emission, emission by a stellar photosphere, or a combination of these. Of the 36 novae detected in one or more WISE bands, 16 are detected in all four; 31 known novae are not detected by WISE. We also searched for WISE data on post-WISE novae, to gain information about nova progenitors. In this first paper, we consider only the WISE data. In future papers, we will provide a more detailed modelling of the WISE data, and discuss WISE data on post-WISE novae – including their variability – and will complement the WISE data with data from other IR surveys.
Citation
(2014). A WISE view of novae - I. The data. Monthly Notices of the Royal Astronomical Society, 1683 - 1697. https://doi.org/10.1093/mnras/stu1467
Acceptance Date | Jul 21, 2014 |
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Publication Date | Oct 21, 2014 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Publisher | Oxford University Press |
Pages | 1683 - 1697 |
DOI | https://doi.org/10.1093/mnras/stu1467 |
Keywords | surveys, binaries, symbiotic, circumstellar matter, novae, cataclysmic variables, infrared, stars |
Publisher URL | https://doi.org/10.1093/mnras/stu1467 |
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