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It is well known that stellar winds are variable, and the
fluctuations are often cyclical in nature. This property seems to
be shared by the winds of cool and hot stars, even though their
outflows are driven by fundamentally different physical mechanisms.
Since very similar models have been proposed to explain the
cyclical wind variations observed in a wide variety of stars, the
time was ripe for astrophysicists from many different
sub-disciplines to present the state of the art in a concise form.
The proceedings will provide a useful, up-to-date overview of the
observations, interpretation, and modelling of the time-dependent
mass outflows from all sorts of stars.
It is well known that stellar winds are variable, and the
fluctuations are often cyclical in nature. This property seems to
be shared by the winds of cool and hot stars, even though their
outflows are driven by fundamentally different physical mechanisms.
Since very similar models have been proposed to explain the
cyclical wind variations observed in a wide variety of stars, the
time was ripe for astrophysicists from many different
sub-disciplines to present the state of the art in a concise form.
The proceedings will provide a useful, up-to-date overview of the
observations, interpretation, and modelling of the time-dependent
mass outflows from all sorts of stars.
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