Using the recently developed CORS method, applied to the photometric data of Walraven et al. (1964), we have determined improved radii for the three classica! cepheids V381 Cen, VSOO Sco, and SV Vel. These new determinations are in good agreement with theoretical computations for the center of the instability strip (Cogan, 1978). Some peculiar parameters are also computed, from the analysis of photometric data.

A reanalysis of the data of three classical cepheids - V381 Cen, V500 Sco, and SV Vel

Guido Russo
Writing – Original Draft Preparation
1983

Abstract

Using the recently developed CORS method, applied to the photometric data of Walraven et al. (1964), we have determined improved radii for the three classica! cepheids V381 Cen, VSOO Sco, and SV Vel. These new determinations are in good agreement with theoretical computations for the center of the instability strip (Cogan, 1978). Some peculiar parameters are also computed, from the analysis of photometric data.
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/11588/892667
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