Analysis of photometry of luminous hot stars from BRITE

Analysis of photometry of luminous hot stars from BRITE

 

M. Rybicka and the BRITE Team

 

The hot part of the Hertzsprung-Russell diagram contains many types of variable stars. The driving mechanisms are not yet understood. They can be pulsations, convection, stellar wind, granulation or other processes. The pulsations can be excited by dierent mechanisms. We will present here the results of the analysis of the BRITE-Constellation photometry of OB stars.

 

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