Buch, Englisch, 488 Seiten, Format (B × H): 175 mm x 250 mm, Gewicht: 1017 g
Buch, Englisch, 488 Seiten, Format (B × H): 175 mm x 250 mm, Gewicht: 1017 g
Reihe: Cambridge Contemporary Astrophysics
ISBN: 978-0-521-87998-9
Verlag: Cambridge University Press
Metal-rich stars accumulate their metals from previous generations of stars, and so contain the history of their galaxy. By studying these stars we can gain valuable insights into how metals change the formation and evolution of stars, and explain the extraordinary massive star populations observed in the metal-rich region of our own galaxy. Recent observations of metal-rich regions have shown that stars hosting giant planets are generally metal-rich, which has triggered further observations of metal-rich stars. This has led to the discovery of new exoplanets, and advances in the study of planet formation and the late chemical evolution of galaxies. This book is the first on this topic, and it covers many aspects, from spectral line formation to stellar formation and evolution in high metallicity regimes. It is invaluable to researchers and graduate students in stellar evolution, extragalactic astronomy, and planet formation.
Autoren/Hrsg.
Fachgebiete
Weitere Infos & Material
Part I. Abundances in the Galaxy; Part II. Abundances in the Galaxy; Part III. Observations - Abundances in Extragalactic Contexts; Part IV. Stellar Populations and Mass Functions; Part V. Physical Processes at High Metallicity; Part VI. Formation and Evolution of Metal-Rich Stars and Stellar Yields; Part VII. Chemical and Photometric Evolution beyond Solar Metallicity.




