An investigation of the variability of V 351 Ori. I - Observations

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Electrophotometry, Stellar Luminosity, Stellar Spectrophotometry, Ubv Spectra, Variable Stars, Spectral Energy Distribution, Spectrum Analysis, Stellar Color

Scientific paper

Photoelectric UBVRI measurements of the brightness of the variable star 351 Ori are presented. The observations were carried out in the course of 103 nights using the AZT-14 telescope of the Main Astrophysical Observatory of the Ukrainian Academy of Sciences attached to a AEF-2 electrophotometer. Analysis of the electrophotometric data revealed evidence of quiet and active periods of light variation. In the normal state, the amplitude of the variations was 0.3 m; weakening of the variability of violet light by about 2 m was also observed. It is shown that the weakening periods were also accompanied by color changes.

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