Variations of HD 137509 (Mathys+ 1997)

Physics

Scientific paper

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Stars: Bp, Photometry: Geneva

Scientific paper

A refined value P=(4.4916+/-0.0002) d is derived for the rotation period of the Bp star HD 137509, from the simultaneous consideration of photometric data recorded in the Geneva system and of measurements of the mean longitudinal magnetic field and of the crossover. The photometric data are given in Table 1. For a description of the Geneva photometric system, see e.g. (1 data file).

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