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Synopsis
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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The Origin of Outflows in Evolved Stars (IAU S366): Proceedings of the 366th Symposium of the International Astronomical Union Virtual Meeting, . Astronomical Union Symposia and Colloquia)
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The Origin of Outflows in Evolved Stars (IAU S366) (Hardcover)
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Hardcover. Etat : new. Hardcover. 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. All stars are known to power strong stellar winds at the end of their lives, expelling stellar material that is recycled as building blocks of new planets and life. IAU S366 provides an overview of state-of-the-art observational, theoretical and numerical studies on the origin of winds in evolved stars. Shipping may be from multiple locations in the US or from the UK, depending on stock availability. N° de réf. du vendeur 9781108490795
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The Origin of Outflows in Evolved Stars (IAU S366) (Proceedings of the International Astronomical Union Symposia and Colloquia)
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The Origin of Outflows in Evolved Stars (Iau S366)
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Etat : New. InhaltsverzeichnisPreface Getting started: how a supersonic stellar wind is initiated from a hydrostatic surface The first 3D models of evolved hot star outflows The origin and impact of Wolf-Rayet-type mass loss Magnetised gas nebul. N° de réf. du vendeur 692082174
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The Origin of Outflows in Evolved Stars: Proceedings of the 366th Symposium of the International Astronomical Union Virtual Meeting, Initially Planned for Leuven Belgium 1-6 November, 2021
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The Origin of Outflows in Evolved Stars: Proceedings of the 366th Symposium of the International Astronomical Union Virtual Meeting, Initially Planned . 2021 (IAU Symposium Proceedings Series)
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The Origin of Outflows in Evolved Stars: Proceedings of the 366th Symposium of the International Astronomical Union Virtual Meeting, Initially Planned . 2021 (IAU Symposium Proceedings Series)
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The Origin of Outflows in Evolved Stars (IAU S366)
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Buch. Etat : Neu. Neuware - 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. N° de réf. du vendeur 9781108490795
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