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dc.contributor.advisorPhilip Morrison.en_US
dc.contributor.authorSeals, Rupert LaWendellen_US
dc.contributor.otherMassachusetts Institute of Technology. Dept. of Physics.en_US
dc.date.accessioned2012-01-12T18:31:39Z
dc.date.available2012-01-12T18:31:39Z
dc.date.copyright1982en_US
dc.date.issued1982en_US
dc.identifier.urihttp://hdl.handle.net/1721.1/68225
dc.descriptionThesis (M.S.)--Massachusetts Institute of Technology, Dept. of Physics, 1982.en_US
dc.descriptionMICROFICHE COPY AVAILABLE IN ARCHIVES AND SCIENCEen_US
dc.descriptionBibliography: leaves 29-30.en_US
dc.description.statementofresponsibilityby Rupert LaWendell Seals.en_US
dc.format.extent48 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.subjectPhysics.en_US
dc.subject.lcshX-ray sources, Galacticen_US
dc.subject.lcshGalaxiesen_US
dc.subject.lcshStarsen_US
dc.titleModelling of M82 and NGC7714 star burst cores using x-ray emitting objectsen_US
dc.typeThesisen_US
dc.description.degreeM.S.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.identifier.oclc10380551en_US


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