Application of radiative hydrodynamics to the problem of mass loss from red giant stars

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dc.contributor.advisorKwok, Sun
dc.contributor.authorZhang, Guojin
dc.date.accessioned2005-07-29T21:35:27Z
dc.date.available2005-07-29T21:35:27Z
dc.date.issued1996
dc.descriptionBibliography: p. 111-117.en
dc.format.extentxvi, 117 leaves ; 30 cm.en
dc.identifier.citationZhang, G. (1996). Application of radiative hydrodynamics to the problem of mass loss from red giant stars (Master's thesis, University of Calgary, Calgary, Canada). Retrieved from https://prism.ucalgary.ca. doi:10.11575/PRISM/16501en_US
dc.identifier.doihttp://dx.doi.org/10.11575/PRISM/16501
dc.identifier.isbn0612129101en
dc.identifier.lccQB 843 R42 Z43 1996en
dc.identifier.urihttp://hdl.handle.net/1880/29499
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.subject.lccQB 843 R42 Z43 1996en
dc.subject.lcshRed giants
dc.subject.lcshMass loss (Astrophysics)
dc.titleApplication of radiative hydrodynamics to the problem of mass loss from red giant 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 1071 520538448
ucalgary.thesis.notesUARCen
ucalgary.thesis.uarcreleaseyen
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