BOOKREVIEWS N° R1024
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Published in 2008 by CAMBRIDGE UNIVERSITY PRESS
Address : The Edinburgh
Building, Shaftesbury Road, Cambridge CB2 2RU, UK
Telephone : 01223
312393
Fax : 01223 315052
Internet : www.cambridge.org
ISBN : 978-0-521-8798-9
- 470 pages – hardback
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.
• The first book on the topic
of metal-rich stars • Metal-rich stars are an emerging field in astrophysics,
and are particularly interesting in the context of the study of exoplanets and
planet formation, and also galaxy evolution • Includes recent results and
observations of metal-rich star distributions in the Milky Way and beyond

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