arXiv (OAI Expanded)
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The study of AF And. I. Hydrogen abundance constraints and dynamically-consistent wind model of the hot state
This paper starts a series of works devoted to an in-depth study of luminous blue variable AF And in the M31 galaxy. Here we present the results of non-LTE modelling of the star in a hot state with CMFGEN code. In addition to the $β$-velocity law, widely used in the analysis of stellar atmospheres,
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