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dc.contributor.authorStrugarek, Antoine
dc.contributor.authorBrun, Allan Sacha
dc.contributor.authorMatt, Sean P.
dc.contributor.authorReville, Victor
dc.date.accessioned2016-01-25T09:45:47Z
dc.date.issued2013-06
dc.description.abstractWe model the magnetized interaction between a star and a close-in planet (SPMIs), using global, magnetohydrodynamic numerical simulations. In this proceedings, we study the effects of the numerical boundary conditions at the stellar surface, where the stellar wind is driven, and in the planetary interior. We show that is it possible to design boundary conditions that are adequate to obtain physically realistic, steady-state solutions for cases with both magnetized and unmagnetized planets. This encourages further development of numerical studies, in order to better constrain and undersand SPMIs, as well as their effects on the star-planet rotational evolution. © 2013 International Astronomical Union.en_GB
dc.identifier.citationVol. 8, pp. 330 - 334en_GB
dc.identifier.doi10.1017/S1743921313011162
dc.identifier.urihttp://hdl.handle.net/10871/19343
dc.language.isoenen_GB
dc.publisherCambridge University Pressen_GB
dc.relation.urlhttp://arxiv.org/abs/1311.3902en_GB
dc.subjectMagnetohydrodynamics (MHD)en_GB
dc.subjectOutflowsen_GB
dc.subjectPlanet-star interactionsen_GB
dc.subjectStars: windsen_GB
dc.titleModeling magnetized star-planet interactions: boundary conditions effectsen_GB
dc.typeConference proceedingsen_GB
dc.date.available2016-01-25T09:45:47Z
dc.identifier.issn1743-9213
dc.descriptionConference Proceedingen_GB
dc.descriptionCopyright © International Astronomical Union 2013en_GB
dc.identifier.eissn1743-9221
dc.identifier.journalProceedings of the International Astronomical Unionen_GB


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