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Long time-scale variability of X-ray binaries with late-type giant companions

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dc.contributor.authorFilippova, Ekaterina
dc.contributor.authorRevnivtsev, M.
dc.contributor.authorParkin, Elliott
dc.date.accessioned2015-12-13T22:32:59Z
dc.date.issued2014
dc.date.updated2015-12-11T09:13:03Z
dc.description.abstractIn this paper we propose and examine a physical mechanism which can lead to the generation of noise in themass accretion rate of low-mass X-ray binaries on time-scales comparable to the orbital period of the system.We consider modulations of mass captured
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/75825
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.titleLong time-scale variability of X-ray binaries with late-type giant companions
dc.typeJournal article
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage115
local.bibliographicCitation.startpage108
local.contributor.affiliationFilippova, Ekaterina, Space Research Institute
local.contributor.affiliationRevnivtsev, M. , Space Research Institute
local.contributor.affiliationParkin, Elliott, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidParkin, Elliott, u4959793
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB4811
local.identifier.citationvolume437
local.identifier.doi10.1093/mnras/stt1870
local.identifier.scopusID2-s2.0-84890111181
local.identifier.thomsonID000328373000030
local.type.statusPublished Version

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