Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/18850
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dc.contributor.authorKing, A. R.-
dc.contributor.authorPringle, J. E.-
dc.contributor.authorLivio, M.-
dc.date.accessioned2012-10-24T09:06:03Z-
dc.date.available2012-10-24T09:06:03Z-
dc.date.issued2007-04-21-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2007, 376 (4), pp. 1740-1746-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2381/18850-
dc.identifier.urihttp://mnras.oxfordjournals.org/content/376/4/1740-
dc.description.abstractWe consider observational and theoretical estimates of the accretion disc viscosity parameter α. We find that in thin, fully ionized discs, the best observational evidence suggests a typical range α∼ 0.1–0.4, whereas the relevant numerical simulations tend to derive estimates for α which are an order of magnitude smaller. We discuss possible reasons for this apparent discrepancy.-
dc.publisherRoyal Astronomical Society (RAS)-
dc.rightsThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2007 the authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. Deposited with reference to the publisher’s archiving policy available on the SHERPA/RoMEO website.-
dc.sourceScopus-
dc.source.urihttp://www.scopus.com/home.url-
dc.titleAccretion disc viscosity: How big is alpha?-
dc.typeJournal Article-
dc.identifier.doi10.1111/j.1365-2966.2007.11556.x-
dc.identifier.eissn1365-2966-
dc.description.statusPeer-reviewed-
dc.description.versionPublisher Version-
dc.description.irispid43483-
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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