Unconventional origin of supersoft X-ray emission from a white dwarf binary
Unconventional origin of supersoft X-ray emission from a white dwarf binary
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Author / Creator
Maccarone, Thomas J. , Nelson, Thomas J. , Brown, Peter J. , Mukai, Koji , Charles, Philip A. , Rajoelimanana, Andry , Buckley, David A. H. , Strader, Jay , Chomiuk, Laura , Britt, Christopher T. , Jha, Saurabh W. , Mróz, Przemek , Udalski, Andrzej , Szymański, Michal K. , Soszyński, Igor , Poleski, Radosław , Kozłowski, Szymon , Pietrukowicz, Paweł , Skowron, Jan and Ulaczyk, Krzysztof
Publisher
London: Nature Publishing Group UK
Journal title
Language
English
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Publisher
London: Nature Publishing Group UK
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Scope and Contents
Contents
Supersoft X-ray sources are stellar objects that emit X-rays with temperatures of about 1 million kelvin and luminosities well in excess of what can be produced by stellar coronae. It has generally been presumed that the objects in this class are binary star systems in which mass transfer leads to nuclear fusion on the surface of a white dwarf
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Alternative Titles
Full title
Unconventional origin of supersoft X-ray emission from a white dwarf binary
Authors, Artists and Contributors
Author / Creator
Nelson, Thomas J.
Brown, Peter J.
Mukai, Koji
Charles, Philip A.
Rajoelimanana, Andry
Buckley, David A. H.
Strader, Jay
Chomiuk, Laura
Britt, Christopher T.
Jha, Saurabh W.
Mróz, Przemek
Udalski, Andrzej
Szymański, Michal K.
Soszyński, Igor
Poleski, Radosław
Kozłowski, Szymon
Pietrukowicz, Paweł
Skowron, Jan
Ulaczyk, Krzysztof
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_journals_2389713644
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2389713644
Other Identifiers
ISSN
2397-3366
E-ISSN
2397-3366
DOI
10.1038/s41550-018-0639-1
