Direct analysis of type Ia supernovae spectra.

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dc.contributor.advisorBranch, David,en_US
dc.contributor.authorFisher, Adam Keith.en_US
dc.date.accessioned2013-08-16T12:30:49Z
dc.date.available2013-08-16T12:30:49Z
dc.date.issued2000en_US
dc.description.abstractThis work describes how to use and modify the highly parameterized spectrum synthesis code (SYNNEW). SYNNEW can be used to derive information directly from type Ia supernovae spectra.en_US
dc.format.extentv, 159 leaves :en_US
dc.identifier.urihttp://hdl.handle.net/11244/5920
dc.noteAdviser: David Branch.en_US
dc.noteSource: Dissertation Abstracts International, Volume: 61-02, Section: B, page: 0891.en_US
dc.subjectSupernovae Spectra.en_US
dc.subjectSupernovae.en_US
dc.subjectPhysics, Astronomy and Astrophysics.en_US
dc.subjectRed shift.en_US
dc.thesis.degreePh.D.en_US
dc.thesis.degreeDisciplineHomer L. Dodge Department of Physics and Astronomyen_US
dc.titleDirect analysis of type Ia supernovae spectra.en_US
dc.typeThesisen_US
ou.groupCollege of Arts and Sciences::Homer L. Dodge Department of Physics and Astronomy
ou.identifier(UMI)AAI9962949en_US

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