Dynamical phasing of Type II Cepheids
In this paper we examine the problems of phasing using light curves and offer an alternate technique using the changes in acceleration to establish the zero point. We give astrophysical justification as to why this technique is useful and apply the technique to a selection of Type II Cepheids. We then examine some limitations of the technique which qualify its use.
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|01_McSaveney_Dynamical_phasing_of_Type_II_2005.pdf||332.31 kB||Adobe PDF||Request a copy|
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