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arXiv · 1612.06157

The cataclysmic variable AE Aquarii: B-V colour of the flares

R. K. Zamanov·G. Y. Latev·S. Boeva·S. Ibryamov·G. B. Nikolov·K. A. Stoyanov
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Abstract

We report simultaneous observations of the flaring behaviour of the cataclysmic variable star AE Aqr. The observations are in Johnson B and V bands. The colour-magnitude diagrams (B-V versus V and B-V vs. B) show that the star becomes blues as it becomes brighter. In our model AE Aqr behaviour can be explained with flares (fireballs) with 0.03 < B-V < 0.30 and temperature in the interval 8000 < T < 12000.

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R. K. Zamanov, G. Y. Latev, S. Boeva, S. Ibryamov, G. B. Nikolov, K. A. Stoyanov. 2016-12-19. The cataclysmic variable AE Aquarii: B-V colour of the flares. https://doi.org/10.1002/asna.201713294

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