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dc.contributor.authorKotze, M. M.
dc.contributor.authorCharles, P. A.
dc.date.accessioned2023-01-18T14:25:39Z
dc.date.available2023-01-18T14:25:39Z
dc.date.issued2015
dc.identifier.citationActa Polytechnica. 2015, vol. 2, no. 1, p. 127-132.
dc.identifier.issn1210-2709 (print)
dc.identifier.issn1805-2363 (online)
dc.identifier.urihttp://hdl.handle.net/10467/105768
dc.description.abstractLong term modulations have been detected in a wide variety of both low and high-mass X-ray binaries. The All Sky Monitor on board the Rossi X-ray Timing Explorer provides the most extensive (~15 years) and sensitive X-ray archive for studying such behaviour. Since those variations were often intermittent and/or aperiodic, we used a time-dependent Dynamic Power Spectrum method to examine how the modulations themselves vary with time in a systematic way. Some were found to be remarkably stable, while others show a range of properties, from even longer variability time-scales to quite chaotic behaviour.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherČeské vysoké učení technické v Prazecs
dc.publisherCzech Technical University in Pragueen
dc.relation.ispartofseriesActa Polytechnica
dc.relation.urihttps://ojs.cvut.cz/ojs/index.php/APP/article/view/2859
dc.rightsCreative Commons Attribution 4.0 International Licenseen
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.titleInvestigating Long-Term Behaviour of X-ray Binaries Using Archival Data
dc.typearticleen
dc.date.updated2023-01-18T14:25:39Z
dc.identifier.doi10.14311/APP.2015.02.0128
dc.rights.accessopenAccess
dc.type.statusPeer-reviewed
dc.type.versionpublishedVersion


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Creative Commons Attribution 4.0 International License
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