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dc.contributor.authorGregory, S.G.
dc.contributor.authorHolzwarth, V.R.
dc.contributor.authorDonati, J.-F.
dc.contributor.authorHussain, G.A.J.
dc.contributor.authorMontmerle, T.
dc.contributor.authorAlecian, E.
dc.contributor.authorAlencar, S.H.P.
dc.contributor.authorArgiroffi, C.
dc.contributor.authorAudard, M.
dc.contributor.authorBouvier, J.
dc.contributor.authorDamiani, F.
dc.contributor.authorGüdel, M.
dc.contributor.authorHuenemoerder, D.P.
dc.contributor.authorKastner, J.H.
dc.contributor.authorMaggio, A.
dc.contributor.authorSacco, G.G.
dc.contributor.authorWade, G.A.
dc.date.accessioned2014-07-08T16:01:04Z
dc.date.available2014-07-08T16:01:04Z
dc.date.issued2014-01-08
dc.identifier.citationGregory , S G , Holzwarth , V R , Donati , J-F , Hussain , G A J , Montmerle , T , Alecian , E , Alencar , S H P , Argiroffi , C , Audard , M , Bouvier , J , Damiani , F , Güdel , M , Huenemoerder , D P , Kastner , J H , Maggio , A , Sacco , G G & Wade , G A 2014 , ' The magnetosphere of the close accreting PMS binary V4046 Sgr ' , EPJ Web of Conferences , vol. 64 , 08009 . https://doi.org/10.1051/epjconf/20136408009en
dc.identifier.issn2100-014X
dc.identifier.otherPURE: 130510651
dc.identifier.otherPURE UUID: ceb32c6f-e5a9-4a28-9885-d728ec0ece5b
dc.identifier.otherScopus: 84893561829
dc.identifier.otherWOS: 000342352600056
dc.identifier.urihttp://hdl.handle.net/10023/4974
dc.descriptionSGG acknowledges support from the Science & Technology Facilities Council (STFC) via an Ernest Rutherford Fellowship [ST/J003255/1]. GAW is supported by a Discovery Grant from the Natural Science & Engineering Research Council of Canada (NSERC).en
dc.description.abstractV4046 Sagittarii AB is a close short-period classical T Tauri binary. It is a circularised and synchronised system accreting from a circumbinary disk. In 2009 it was observed as part of a coordinated program involving near-simultaneous spectropolarimetric observations with ESPaDOnS at the Canada-France-Hawai'i Telescope and high-resolution X-ray observations with XMM-Newton. Magnetic maps of each star were derived from Zeeman-Doppler imaging. After briefly highlighting the most significant observational findings, we present a preliminary 3D model of the binary magnetosphere constructed from the magnetic maps using a newly developed binary magnetic field extrapolation code. The large-scale fields (the dipole components) of both stars are highly tilted with respect to their rotation axes, and their magnetic fields are linked.
dc.format.extent4
dc.language.isoeng
dc.relation.ispartofEPJ Web of Conferencesen
dc.rights© Owned by the authors, published by EDP Sciences, 2014. This is an Open Access article distributed under the terms of the Creative Commons Attribution License 2.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. http://creativecommons.org/licenses/by/2.0/en
dc.subjectQC Physicsen
dc.subject.lccQCen
dc.titleThe magnetosphere of the close accreting PMS binary V4046 Sgren
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.The University of St Andrewsen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1051/epjconf/20136408009
dc.description.statusPeer revieweden
dc.identifier.urlhttp://www.epj-conferences.org/articles/epjconf/abs/2014/01/epjconf_mag2013_08009/epjconf_mag2013_08009.htmlen


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