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Photometric variability of
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Wolf-Rayet type star HD 191765
Nowadays, the application of photometers equipped with modern light receivers (CCD - Charge Coupled Device) in photometric observations and the use of more modern mathematical analysis methods in the processing of photometric CCD images of stars allow more accurate investigation of the physical processes taking place in stars. This allows us to build more accurate models of the physical processes taking place in stars. It is clear from this that even previously studied stars need to be re-examined with modern astronomical instruments.
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