Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/45144
Title: Neil Gehrels Swift Observatory studies of supersoft novae
Authors: Page, K. L.
Beardmore, A. P.
Osborne, J. P.
First Published: 2019
Publisher: Elsevier for Pergamon, Committee on Space Research (COSPAR)
Citation: Advances in Space Research, Special Issue: "Nova Eruptions, Cataclysmic Variables and Related Systems: observational vs theoretical challenges in the 2020 era", following COSPAR 2018, 2019, In Press
Abstract: The rapid response capabilities of the Neil Gehrels Swift Observatory, together with the daily planning of its observing schedule, make it an ideal mission for following novae in the X-ray and UV bands, particularly during their early phases of rapid evolution and throughout the supersoft source interval. Many novae, both classical and recurrent, have been extensively monitored by Swift throughout their supersoft phase and later decline. We collect here results from observations of novae with outbursts which occurred between the start of 2006 and the end of 2017.
DOI Link: TBA
eISSN: 1879-1948
Links: TBA
http://hdl.handle.net/2381/45144
Embargo on file until: 1-Jan-10000
Version: Post-print
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © Elsevier for Pergamon, Committee on Space Research (COSPAR) 2019. After an embargo period this version of the paper will be an open-access article distributed under the terms of the Creative Commons Attribution-Non Commercial-No Derivatives License (http://creativecommons.org/licenses/by-nc-nd/4.0/), which permits use and distribution in any medium, provided the original work is properly cited, the use is non-commercial and no modifications or adaptations are made.
Description: 54 pages, 33 figure panels, 2 tables. To be published in a Special Issue of Advances in Space Research, entitled "Nova Eruptions, Cataclysmic Variables and Related Systems: observational vs theoretical challenges in the 2020 era", following COSPAR 2018
The file associated with this record is under embargo until 12 months after publication, in accordance with the publisher's self-archiving policy. The full text may be available through the publisher links provided above.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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