Abstract
Using the recently developed CORS method, applied to the photometric data of Walravenet al. (1964), we have determined improved radii for the three classical cepheids V381 Cen, V500 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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Russo, G. A reanalysis of the data of three classical cepheids: V381 Cen, V500 Sco, and SV Vel. Astrophys Space Sci 90, 147–151 (1983). https://doi.org/10.1007/BF00651555
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DOI: https://doi.org/10.1007/BF00651555