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dc.contributor.authorPrice, RHen_US
dc.contributor.authorMarkakis, Cen_US
dc.contributor.authorFriedman, JLen_US
dc.date.accessioned2018-11-29T11:55:19Z
dc.date.issued2009-07en_US
dc.date.submitted2018-11-19T15:50:54.888Z
dc.identifier.issn0022-2488en_US
dc.identifier.other10.1063/1.3166136
dc.identifier.otherARTN 073505en_US
dc.identifier.otherARTN 073505en_US
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/53421
dc.description16 pages, 3 figures
dc.description.sponsorshipWe gratefully acknowledge support for this work under NSF Grant Nos. PHY-0554367 and PHY-0503366, NASA Grant No. NNG05GB99G, by the Greek State Scholarships Foundation, and by the Center for Gravitational Wave Astronomy. Wen_US
dc.language.isoenen_US
dc.relation.ispartofJOURNAL OF MATHEMATICAL PHYSICSen_US
dc.rightsThis is a pre-copyedited, author-produced version of an article accepted for publication in Journal of Mathematical Physics following peer review. The version of record is available https://aip.scitation.org/doi/10.1063/1.3166136
dc.subjectastrophysical fluid dynamicsen_US
dc.subjectbinary starsen_US
dc.subjecteigenvalues and eigenfunctionsen_US
dc.subjectequations of stateen_US
dc.subjectgravitationen_US
dc.subjectiterative methodsen_US
dc.subjectstellar modelsen_US
dc.subjectstellar rotationen_US
dc.subjectstellar structureen_US
dc.titleIteration stability for simple Newtonian stellar systemsen_US
dc.typeArticle
dc.rights.holder© 2009 American Institute of Physics
dc.identifier.doi10.1063/1.3166136en_US
pubs.author-urlhttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000268614500024&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6aen_US
pubs.issue7en_US
pubs.notesNot knownen_US
pubs.publication-statusPublisheden_US
pubs.volume50en_US


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