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    The variable RS Cassicpeiae (108.1904)

    Haynes, Eli Stuart
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    [PDF] VariableRsCassiopeiae.pdf (10.60Mb)
    Date
    1907
    Format
    Thesis
    Metadata
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    Abstract
    The 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.
    URI
    https://hdl.handle.net/10355/15487
    https://doi.org/10.32469/10355/15487
    Degree
    M.A.
    Thesis Department
    Astronomy (MU)
    Rights
    OpenAccess.
    This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivs 3.0 License.
    Collections
    • 1900-1909 Theses (MU)
    • Physics and Astronomy electronic theses and dissertations (MU)

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