Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/36515
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dc.contributor.authorNorton, A. J.-
dc.contributor.authorHellier, C.-
dc.contributor.authorBeardmore, Andrew P.-
dc.contributor.authorWheatley, P. J.-
dc.contributor.authorOsborne, Julian Paul-
dc.contributor.authorTaylor, P.-
dc.date.accessioned2016-02-02T12:18:23Z-
dc.date.available2016-02-02T12:18:23Z-
dc.date.issued1997-08-01-
dc.identifier.citationMonthly Notices Of The Royal Astronomical Society, 1997, 289 (2), pp. 362-370 (9)en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://mnras.oxfordjournals.org/content/289/2/362.shorten
dc.identifier.urihttp://hdl.handle.net/2381/36515-
dc.description.abstractWe report on two recent X-ray observations of the intermediate polar TX Col made with ASCA and ROSAT. From a consideration of the power spectra of their light curves, we show that the system was accreting predominantly via a disc in 1994 October, but had reverted to a discoverflow mode of accretion by 1995 October, at which time a substantial amount of the accretion was directly via a stream. We discuss possible reasons for this change. By considering the relative phases of the spin and beat pulsations seen in the ROSAT data, as well as their orbital harmonics, we demonstrate that the stream-fed accretion regions on the white dwarf surface remain fixed at about orbital phase 0.7, and thus migrate around the white dwarf. We suggest that the observed orbital modulation results from a combination of two effects: first, attenuation of emission sites by material located at the stream-disc boundary at orbital phase 0.8, and, secondly, the changing visibility of the stream-fed accretion sites which are always on the side of the white dwarf facing the stream.en
dc.language.isoenen
dc.publisherBlackwell Science Ltden
dc.rightsCopyright © 1997 the authors. Monthly Notices of the Royal Astronomical Society © 1997 RAS. All rights reserved. Deposited with reference to the publisher’s archiving policy available on the SHERPA/RoMEO website.en
dc.subjectScience & Technologyen
dc.subjectPhysical Sciencesen
dc.subjectAstronomy & Astrophysicsen
dc.subjectASTRONOMY & ASTROPHYSICSen
dc.subjectaccretion, accretion discsen
dc.subjectstars, individual, TX Colen
dc.subjectstars, individual, H0542-407en
dc.subjectnovae, cataclysmic variablesen
dc.subjectX-rays, starsen
dc.subjectRAY LIGHT-CURVESen
dc.subjectX-RAYen
dc.subjectINTERMEDIATE POLARSen
dc.subjectCATACLYSMIC VARIABLESen
dc.subjectFO AQUARIIen
dc.subjectSPECTRUMen
dc.subjectASCAen
dc.titleStream-fed and disc-fed accretion in TX Columbaeen
dc.typeJournal Articleen
dc.identifier.doi10.1093/mnras/289.2.362-
dc.identifier.eissn1365-2966-
dc.description.statusPeer-revieweden
dc.description.versionPublisher Versionen
dc.type.subtypeArticle;Journal-
pubs.organisational-group/Organisationen
pubs.organisational-group/Organisation/COLLEGE OF SCIENCE AND ENGINEERINGen
pubs.organisational-group/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomyen
dc.dateaccepted1996-12-13-
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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