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dc.contributor.authorHaynes, Eli Stuarten
dc.date.issued1907
dc.descriptionItem taken from Bulletin no 11 of the Laws Observatory Includes a letter (inserted) from the author to Prof Isador Loeb, the Chairman of the Graduate Committee, asking that this paper be accepted " as a thesis in partial satisfaction of the requirements for the degree of Master of Arts"
dc.descriptionM.A. University of Missouri 1907
dc.description.abstractThe variability of this star was discovered by Madame Ceraski from plates made by Blakjo at Moscow, and was announced in A. N. No. 3953. The photographs indicated a variation from the ninth to the eleventh magnitude approximately. Observations by Miss Whitney at the Vassar College Observatory, A. N. No. 4050, confirmed the variation and gave a range in brightness of 9.m7 to 10.m4. The following provisional elements, based upon observations made here, were announced in Laws Observatory Bulletin No. 10. Min. = J.D.2417412.50 + 6.d298E, G.M.T. The present paper contains a revision these elements and a discussion of all the observations thus far obtained.
dc.description.digitizationDigitized at the University of Missouri--Columbia MU Libraries Digitization Lab in 2011.
dc.format.extentp. 167-180
dc.identifier.merlinb23572309
dc.identifier.oclc25284202
dc.identifier.urihttp://hdl.handle.net/10355/15487
dc.publisherUniversity of Missouri
dc.relation.ispartofTheses and Dissertations (MU)
dc.relation.ispartofcommunityUniversity of Missouri-Columbia. Libraries. MU Libraries Locally Digitized Materials
dc.subject.lcshVariable stars
dc.titleThe variable RS Cassicpeiae (108.1904)en
dc.typeThesis
thesis.degree.disciplineAstronomyeng
thesis.degree.grantorUniversity of Missouri--Columbiaeng
thesis.degree.grantorUniversity of Missouri
thesis.degree.levelM.A.
thesis.degree.nameMasters


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