WW Vul B light curve during 1898-1966 (Friedemann+ 1996)

Physics

Scientific paper

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Stars: Variable, Photometry

Scientific paper

Photographic magnitudes are presented for the irregular variable WW
Vulpeculae. They were derived from Argelander brightness estimates
carried out on N=2774 plates of the Harvard College Observatory Plate
Collection. The data set covers the period 1898 to 1966. (1 data file).

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