A new model for soft gamma-ray repeaters and anomalous x-ray pulsars using quark stars

dc.contributor.advisorLeahy, David A.
dc.contributor.authorNiebergal, Brian Phillip
dc.date.accessioned2017-12-18T21:16:14Z
dc.date.available2017-12-18T21:16:14Z
dc.date.issued2007
dc.descriptionBibliography: p. 146-154en
dc.format.extentxiii, 154 leaves : ill. ; 30 cm.en
dc.identifier.citationNiebergal, B. P. (2007). A new model for soft gamma-ray repeaters and anomalous x-ray pulsars using quark stars (Master's thesis, University of Calgary, Calgary, Canada). Retrieved from https://prism.ucalgary.ca. doi:10.11575/PRISM/830en_US
dc.identifier.doihttp://dx.doi.org/10.11575/PRISM/830
dc.identifier.urihttp://hdl.handle.net/1880/101831
dc.language.isoeng
dc.publisher.institutionUniversity of Calgaryen
dc.publisher.placeCalgaryen
dc.rightsUniversity of Calgary graduate students retain copyright ownership and moral rights for their thesis. You may use this material in any way that is permitted by the Copyright Act or through licensing that has been assigned to the document. For uses that are not allowable under copyright legislation or licensing, you are required to seek permission.
dc.titleA new model for soft gamma-ray repeaters and anomalous x-ray pulsars using quark stars
dc.typemaster thesis
thesis.degree.disciplinePhysics and Astronomy
thesis.degree.grantorUniversity of Calgary
thesis.degree.nameMaster of Science (MSc)
ucalgary.thesis.accessionTheses Collection 58.002:Box 1741 520492258
ucalgary.thesis.notesUARCen
ucalgary.thesis.uarcreleaseyen
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