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dc.contributor.authorPratt, John Paul, 1945-
dc.creatorPratt, John Paul, 1945-en_US
dc.date.accessioned2013-05-09T09:56:46Z
dc.date.available2013-05-09T09:56:46Z
dc.date.issued1976en_US
dc.identifier.urihttp://hdl.handle.net/10150/289405
dc.language.isoen_USen_US
dc.publisherThe University of Arizona.en_US
dc.rightsCopyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author.en_US
dc.subjectDouble stars.en_US
dc.titleTHE DEPENDENCE OF THEORETICAL BINARY STAR MASS TRANSFER RATES ON THE ASSUMPTION OF SYNCHRONOUS ROTATIONen_US
dc.typetexten_US
dc.typeDissertation-Reproduction (electronic)en_US
dc.identifier.oclc2602140en_US
thesis.degree.grantorUniversity of Arizonaen_US
thesis.degree.leveldoctoralen_US
dc.identifier.proquest7621101en_US
thesis.degree.disciplineGraduate Collegeen_US
thesis.degree.disciplineAstronomyen_US
thesis.degree.namePh.D.en_US
dc.identifier.bibrecord.b18152685en_US
refterms.dateFOA2018-06-05T23:25:11Z


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