IAU S366 provides an overview of state-of-the-art observational and theoretical studies on the origin of winds in evolved stars.
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Seller: WeBuyBooks, Rossendale, LANCS, United Kingdom
hardcover. Condition: Like New. Most items will be dispatched the same or the next working day. An apparently unread copy in perfect condition. Dust cover is intact with no nicks or tears. Spine has no signs of creasing. Pages are clean and not marred by notes or folds of any kind. Seller Inventory # rev2158185613
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Seller: Grand Eagle Retail, Bensenville, IL, U.S.A.
Hardcover. Condition: 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. Seller Inventory # 9781108490795
Seller: California Books, Miami, FL, U.S.A.
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Seller: moluna, Greven, Germany
Condition: 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. Seller Inventory # 692082174
Seller: Revaluation Books, Exeter, United Kingdom
Hardcover. Condition: Brand New. 400 pages. 10.00x7.09x0.75 inches. In Stock. Seller Inventory # x-1108490794
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Seller: Books Puddle, New York, NY, U.S.A.
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Seller: Majestic Books, Hounslow, United Kingdom
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Seller: AHA-BUCH GmbH, Einbeck, Germany
Buch. Condition: 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. Seller Inventory # 9781108490795