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Modelling of M82 and NGC7714 star burst cores using x-ray emitting objects

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dc.contributor.advisor Philip Morrison. en_US
dc.contributor.author Seals, Rupert LaWendell en_US
dc.contributor.other Massachusetts Institute of Technology. Dept. of Physics. en_US
dc.date.accessioned 2012-01-12T18:31:39Z
dc.date.available 2012-01-12T18:31:39Z
dc.date.copyright 1982 en_US
dc.date.issued 1982 en_US
dc.identifier.uri http://hdl.handle.net/1721.1/68225
dc.description Thesis (M.S.)--Massachusetts Institute of Technology, Dept. of Physics, 1982. en_US
dc.description MICROFICHE COPY AVAILABLE IN ARCHIVES AND SCIENCE en_US
dc.description Bibliography: leaves 29-30. en_US
dc.description.statementofresponsibility by Rupert LaWendell Seals. en_US
dc.format.extent 48 leaves en_US
dc.language.iso eng en_US
dc.publisher Massachusetts Institute of Technology en_US
dc.rights M.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.uri http://dspace.mit.edu/handle/1721.1/7582 en_US
dc.subject Physics. en_US
dc.subject.lcsh X-ray sources, Galactic en_US
dc.subject.lcsh Galaxies en_US
dc.subject.lcsh Stars en_US
dc.title Modelling of M82 and NGC7714 star burst cores using x-ray emitting objects en_US
dc.type Thesis en_US
dc.description.degree M.S. en_US
dc.contributor.department Massachusetts Institute of Technology. Dept. of Physics. en_US
dc.identifier.oclc 10380551 en_US


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