stee philippe (5 Ergebnisse)

Hardcover. Zustand: Like New. First Edition. Firm and square with strong joints, just showing a few very minor rubs and bumps. Hence a non-text page is stamped 'damaged'. Despite such this book is actually in nearly new condition. Thus it looks and feels unread with contents that are crisp, fresh and tight. Size: 255mm x 180mm. Pages: xix, 507. Illustrated and fully indexed. This book provides an introduction to the techniques used to investigate the properties of massive stars, including asteroseismology, spectropolarimetry, and interferometry. It highlights synergies between these new techniques and more classical methods, to create a synthetic view of massive stars, leading researchers towards new and innovative solutions to the most topical questions regarding the evolution of massive stars.

Zustand: New. In.

Zustand: New. A summary of new and innovative techniques used to investigate and understand massive stars, for researchers and graduate students. Editor(s): Meynet, Georges; Georgy, Cyril; Groh, Jose; Stee, Philippe. Series: Proceedings of the International Astronomical Union Symposia and Colloquia. Num Pages: 500 pages, 100 b/w illus. BIC Classification: PGM. Category: (U) Tertiary Education (US: College). Dimension: 257 x 184 x 24. Weight in Grams: 1000. . 2015. Illustrated. hardcover. . . . . Books ship from the US and Ireland.

Hardcover. Zustand: Brand New. 1st edition. 500 pages. 10.00x7.00x1.00 inches. In Stock.

Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - Massive stars play a crucial role in the Universe: they are important drivers for the photometric and chemical evolution of galaxies; they are sources of important elements, including those necessary for life; and, with their strong winds and supernova explosions, they feed the interstellar medium with momentum and kinetic energy, impacting on the star formation rate. Knowledge of the evolution of massive stars is important not only for stellar physics, but also for probing the evolution of galaxies and their star formation histories throughout cosmic time. This volume provides an introduction to these topics and to the techniques used to investigate the properties of massive stars, including asteroseismology, spectropolarimetry, and interferometry. It highlights synergies between these new techniques and more classical methods, to create a synthetic view of massive stars, leading researchers towards new and innovative solutions to the most topical questions regarding the evolution of massive stars.