The period of BW Vulpeculae

Details The period of BW Vulpeculae The period of BW Vulpeculae

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...186..129v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 186, no. 1-2, Nov. 1987, p. 129-135. FNRS-supported research.

Astronomy and Astrophysics

Astrophysics

9

Periodic Variations, Spectrum Analysis, Variable Stars, Data Bases, Radiant Flux Density

Scientific paper

The data of the 1982 BW Vul observing campaign are examined for periodicity. A precise redetermination of the period yields P = 0d.2010425±0d.0000007. The presence of other periodicities with amplitudes larger than 0m.01 is excluded. The different shapes of the stillstand phases do not repeat themselves in a periodic way, as far as periods longer than two days are concerned. An independent analysis of the period variation is carried out using historic and new times of minimum light.

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