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- W133020235 abstract "Hot emission stars (Oe and Be stars) present complex spectral line profiles, which are formed by a number of DACs and/or SACs. In order to explain and reproduce theoretically these complex line profiles we use the GR model (Gauss-Rotation model). This model presupposes that the regions, where the spectral lines are created, consist of a number of independent and successive absorbing or emitting density regions of matter. Here we are testing a new approach of the GR model, which supposes that the independent density regions are not successive. We use this new approach in the spectral lines of some Oe and Be stars and we compare the results of this method with the results deriving from the classical GR model that supposes successive regions." @default.
- W133020235 created "2016-06-24" @default.
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- W133020235 date "2010-01-01" @default.
- W133020235 modified "2023-10-17" @default.
- W133020235 title "Studying the location of SACs and DACs regions in the environment of hot emission stars" @default.
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- W133020235 hasPublicationYear "2010" @default.
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