Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/37557
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dc.contributor.authorNixon, Chris J.-
dc.contributor.authorPringle, J. E.-
dc.date.accessioned2016-05-16T08:33:54Z-
dc.date.available2016-05-16T08:33:54Z-
dc.date.issued2010-04-21-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2010, 403 (4), pp. 1887-1893en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://mnras.oxfordjournals.org/content/403/4/1887en
dc.identifier.urihttp://hdl.handle.net/2381/37557-
dc.description.abstractWe consider the response of a protostellar disc to a tidally induced warp and the resultant changes in the spectral energy distribution (SED). We argue that for typical protostellar disc parameters the warp is communicated through the disc in a wave-like fashion. We find that the main effects of the warp tend to be at large radii (R≳ 30 au) and, for sufficiently small viscosity, can be quite long-lived. This can result in non-uniform illumination of the disc at these radii and can induce significant changes to the SED at wavelengths λ≳ 100 μm.en
dc.language.isoenen
dc.publisherOxford University Press on behalf of the Royal Astronomical Societyen
dc.rightsThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. Copyright © 2010 the authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.en
dc.subjectScience & Technologyen
dc.subjectPhysical Sciencesen
dc.subjectAstronomy & Astrophysicsen
dc.subjectASTRONOMY & ASTROPHYSICSen
dc.subjectaccretion, accretion discsen
dc.subjectstars: formationen
dc.subjectstars: pre-main-sequenceen
dc.subjectSPECTRAL ENERGY-DISTRIBUTIONSen
dc.subjectT-TAURI STARSen
dc.subjectHERBIG AE/BE STARSen
dc.subjectACCRETION DISKSen
dc.subjectNUMERICAL SIMULATIONSen
dc.subjectPROTOPLANETARY DISKSen
dc.subjectCIRCUMSTELLAR DISKSen
dc.subjectINNER HOLEen
dc.subjectENCOUNTERSen
dc.subjectAPPEARANCEen
dc.titleThe observable effects of tidally induced warps in protostellar discsen
dc.typeJournal Articleen
dc.identifier.doi10.1111/j.1365-2966.2010.16331.x-
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.dateaccepted2009-12-23-
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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