PR and PL (PMv) relations for classical Cepheids revisited

Using observational data available for a large number of Galactic Cepheids, we determine the relation between the radius and the period of pulsations, by means of a variant of the Baade-Wesselink method. Using, further, the brightness parameter according to the Barnes-Evans approach, we achieve our...

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Bibliographic Details
Main Authors: Šegan S., Glišović P.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2009-01-01
Series:Serbian Astronomical Journal
Subjects:
Online Access:http://www.doiserbia.nb.rs/img/doi/1450-698X/2009/1450-698X0979101S.pdf