Photoelectric photometry of the Beta Cephei star BW Vulpeculae (1988-1991)

Details Photoelectric photometry of the Beta Cephei star BW Vulpeculae (1988-1991) Photoelectric photometry of the Beta Cephei star BW Vulpeculae (1988-1991)

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as...98..383s&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 98, no. 2, p. 383-389.

Astronomy and Astrophysics

Astrophysics

6

Astronomical Photometry, Cepheid Variables, Electrophotometers, Light Curve, Phase Diagrams, Stellar Oscillations

Scientific paper

BW Vul, the Beta Cephei star with the largest-known amplitude, has been observed through several cycles of pulsation. The data, obtained at three observatories, were homogenized, and are presented in tabular form. Times of minimum and maximum light were derived, and a contemporary value for the period is deduced. Our data do not reveal any sudden period change in the time span 1988-1991.

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