Wind Inhomogeneity is a stellar astrophysical phenomenon characterized by spatial and temporal variations in the density, velocity, and ionization structure of a star's outflowing wind, distinguishing it from uniformly distributed mass loss models.
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J. Puls, N. Markova, Salvatore Scuderi et al. · Astronomy and Astrophysics · 2006 · 261 citations · Full text
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Sofia, Bulgaria
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