BOOKREVIEWS N° R1021
Published in Dec 2007 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 : 978-0-521-87470-0- 588 pages –
hardback
The understanding and
modeling of the structure and evolution of stars is based on statistical
physics as well as on hydrodynamics. Today, a precise identification and proper
description of the physical processes at work in stellar interiors are still lacking
(one key point being that of transport processes) while the comparison of real
stars to model predictions, which implies conversions from the theoretical
space to the observational one, suffers from uncertainties in model
atmospheres. That results in uncertainties on the prediction of stellar
properties needed for galactic studies or cosmology (as stellar ages and
masses). In the next decade, progress is expected from the theoretical,
experimental and observational sides. I illustrate some of the problems we are
faced with when modeling stars and the possible tracks towards their solutions.
I discuss how future observational ground-based or spatial programs (in
particular those dedicated to micro-arc-second astrometry, asteroseismology and
interferometry) will provide precise determinations of the stellar parameters
and contribute to a better knowledge of stellar interiors and atmospheres in a
wide range of stellar masses, chemical compositions and evolution stages.

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