Sprache: Englisch
Verlag: Cambridge University Press, 2023
ISBN 10: 1108490794 ISBN 13: 9781108490795
Anbieter: Prior Books Ltd, Cheltenham, Vereinigtes Königreich
Erstausgabe
EUR 53,76
Anzahl: 2 verfügbar
In den WarenkorbHardcover. Zustand: Like New. First Edition. A firm and square hardback with sharp corners and strong joints, just showing a few very minor cosmetic rubs. Hence a non-text page has a small 'damaged' stamp. Despite such this book is actually in nearly new condition and appears unread. Thus the contents are crisp, fresh and tight; no pen-marks. Now offered for sale at a very sensible price.
Sprache: Englisch
Verlag: Cambridge University Press, 2023
ISBN 10: 1108490794 ISBN 13: 9781108490795
Anbieter: PBShop.store US, Wood Dale, IL, USA
HRD. Zustand: New. New Book. Shipped from UK. Established seller since 2000.
Sprache: Englisch
Verlag: Cambridge University Press, 2023
ISBN 10: 1108490794 ISBN 13: 9781108490795
Anbieter: PBShop.store UK, Fairford, GLOS, Vereinigtes Königreich
EUR 136,76
Anzahl: 2 verfügbar
In den WarenkorbHRD. Zustand: New. New Book. Shipped from UK. Established seller since 2000.
Anbieter: Revaluation Books, Exeter, Vereinigtes Königreich
EUR 141,09
Anzahl: 1 verfügbar
In den WarenkorbHardcover. Zustand: Brand New. 400 pages. 10.00x7.09x0.75 inches. In Stock.
Zustand: 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.
Anbieter: Revaluation Books, Exeter, Vereinigtes Königreich
EUR 192,88
Anzahl: 2 verfügbar
In den WarenkorbHardcover. Zustand: Brand New. 400 pages. 10.00x7.09x0.75 inches. In Stock.
Sprache: Englisch
Verlag: Cambridge University Press Mär 2023, 2023
ISBN 10: 1108490794 ISBN 13: 9781108490795
Anbieter: AHA-BUCH GmbH, Einbeck, Deutschland
Buch. Zustand: 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.
Sprache: Niederländisch
Verlag: Lannoo Campus / Metaforum ku leuven, 2015
ISBN 10: 9401426325 ISBN 13: 9789401426329
Couverture rigide. Zustand: bon. R320181189: 2015. In-8. Relié. Bon état, Couv. convenable, Dos satisfaisant, Intérieur frais. 581 pages - signet conservé - ouvrage en néerlandais. . . . Classification Dewey : 430-Langues germaniques. Allemand.