The Cape rapidly oscillating Ap star survey

 

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dc.contributor.advisor Kurtz, D W en_ZA
dc.contributor.author Martinez, Peter en_ZA
dc.date.accessioned 2015-11-13T13:06:32Z
dc.date.available 2015-11-13T13:06:32Z
dc.date.issued 1993 en_ZA
dc.identifier.citation Martinez, P. 1993. The Cape rapidly oscillating Ap star survey. University of Cape Town. en_ZA
dc.identifier.uri http://hdl.handle.net/11427/14966
dc.description Bibliography: p. 321-330. en_ZA
dc.description.abstract This thesis describes a survey, the Cape Survey, which was started with the intention of discovering more roAp stars suitable for asteroseismological studies and also to identify the limits of the roAp phenomenon in temperature and luminosity. This is the most extensive survey of the roAp phenomenon to date. Prior to the start of the Cape Survey, only 14 roAp stars, discovered over a period of 12 years, were known. The Cape Survey has yielded another 10 new roAp stars in the past three years. The candidates for the Cape Survey were mostly drawn from the Ap SrCrEu stars in the Michigan Spectral Catalogue. en_ZA
dc.language.iso eng en_ZA
dc.subject.other Astronomy en_ZA
dc.title The Cape rapidly oscillating Ap star survey en_ZA
dc.type Thesis / Dissertation en_ZA
uct.type.publication Research en_ZA
uct.type.resource Thesis en_ZA
dc.publisher.institution University of Cape Town
dc.publisher.faculty Faculty of Science en_ZA
dc.publisher.department Department of Astronomy en_ZA
dc.type.qualificationlevel Doctoral en_ZA
dc.type.qualificationname PhD en_ZA
uct.type.filetype Text
uct.type.filetype Image


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