PR and PL (PM_V) 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...
Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
Astronomical Observatory, Department of Astronomy, Belgrade
2009-12-01
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Series: | Serbian Astronomical Journal |
Subjects: | |
Online Access: | http://saj.matf.bg.ac.rs/179/pdf/101-106.pdf |