BOOKREVIEWS
N° R1031
Author :Peter S. Conti , Paul Crowther ,
Claus Leitherer
Published in Oct 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 : 978-0-521-79134-2
- 315 pages – hardback
Luminous hot
stars represent the extreme upper mass end of normal stellar evolution. Before
exploding as supernovae, they live out their lives of a few million years with
prodigious outputs of radiation and stellar winds, dramatically affecting both
their evolution and environments. A detailed introduction to the topic, this
book connects the astrophysics of massive stars with the extremes of galaxy
evolution represented by starburst phenomena. A thorough discussion of the physical
and wind parameters of massive stars is presented. HII galaxies, their
connection to starburst galaxies, and the contribution of starburst phenomena
to galaxy evolution through superwinds, are explored. The book concludes with
the wider cosmological implications, including Population III stars, Lyman
break galaxies and gamma-ray bursts, for each of which massive stars are
believed to play a crucial role. This book is ideal for graduate students and
researchers in astrophysics interested in luminous hot stars and galaxy
evolution.
• The first
book to bring together the astrophysics of luminous hot stars and starburst
galaxies • Presents the latest developments in a diverse but interrelated range
of topics in astrophysics • Will interest graduate students and researchers in
hot star atmospheres, massive star evolution, star and cluster formation,
starburst evolution and superwinds

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