Free Access
Issue
Astron. Astrophys. Suppl. Ser.
Volume 120, Number 3, December_II 1996
Page(s) 429 - 430
DOI https://doi.org/10.1051/aas:1996305
Published online 15 December 1996
WW Vulpeculae: Photographic magnitudes based on plates of the Harvard Plate Collection DOI: 10.1051/aas:1996305

Astronomy and Astrophysics Supplement Series, Vol. 120, December II 1996, 429-430

WW Vulpeculae: Photographic magnitudes based on plates of the Harvard Plate Collection

C. Friedemann, H.-G. Reimann and J. Gürtler
Send offprint requests to: C. Friedemann

Universitäts--Sternwarte, Schillergäßchen 2, D--07745 Jena, Germany

Received April 15; accepted April 16, 1996

Abstract:

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 is available at the CDS and covers the period 1898 to 1966. Although the accuracy of the magnitudes is not high, the data may be useful for the study of the long-term behaviour of the light variations of the variable.

Key words: stars: individual: WW Vul --- stars: variables: other --- circumstellar matter

Tables available in electronic form at the CDS in Strasbourg



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