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The Origin of Outflows in Evolved Stars (IAU S366) (Hardcover)
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The Origin of Outflows in Evolved Stars (IAU S366) (Hardcover)
Series: Proceedings of the International Astronomical Union Symposia and Colloquia
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The prime parameter determining the evolution of a star is its
mass. Any modification to the stellar mass has large repercussions
on its evolutionary path. Both low-mass and massive stars are known
to power strong stellar winds at the end of their lives. These
winds determine the type of the stellar end product and the amount
by which these stars contribute to the chemical enrichment of the
interstellar medium, ultimately providing the building blocks of
planets and life. A proper understanding of stellar evolution and
the building blocks in the Universe cannot be achieved without a
detailed understanding of stellar winds. IAU Symposium 366 provides
an overview of state-of-the-art observational and theoretical
studies on the origin of winds in low-mass and massive evolved
stars, with topics including binarity, enrichment of the
interstellar medium, astrochemistry, and theoretical, observational
and numerical constraints on stellar outflows.
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