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dc.contributor.advisorH. M. Goodwin.en_US
dc.contributor.authorLemaitre, Georges H. J. Een_US
dc.date.accessioned2009-01-30T18:42:27Z
dc.date.available2009-01-30T18:42:27Z
dc.date.issued1927en_US
dc.identifier.urihttp://hdl.handle.net/1721.1/10753
dc.descriptionThesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 1927.en_US
dc.description.statementofresponsibilityby Georges H. J. E. Lemaitre.en_US
dc.format.extent37, [12] leavesen_US
dc.language.isoengen_US
dc.publisherMassachusetts Institute of Technologyen_US
dc.rightsM.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission.en_US
dc.rights.urihttp://dspace.mit.edu/handle/1721.1/7582en_US
dc.subjectPhysicsen_US
dc.titleThe gravitational field in a fluid sphere of uniform invariant density according, to the theory of relativity ; Note on de Sitter ̕Universe ; Note on the theory of pulsating starsen_US
dc.title.alternativeNote on the theory of pulsating starsen_US
dc.typeThesisen_US
dc.description.degreePh.D.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.identifier.oclc36897534en_US


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