
Résumé
Dust is a ubiquitous feature of the cosmos, impinging
directly or indirectly on most fields of modern astronomy
and astrophysics. This book provides a thorough overview of
the subject, covering general concepts, methods of
investigation, important results and their significance,
relevant literature, and some suggestions for promising
avenues of future research.
Since the publication of the first edition of this popular
graduate text, major advances have been made in our
understanding of astrophysical dust, especially in the
light of exciting new results from space and ground-based
telescopes, together with advances in laboratory
astrophysics and theoretical modelling. This new, expanded
edition highlights the latest results and provides a
context for future research opportunities.
The first chapter provides a historical perspective for
current research, together with an overview of interstellar
environments and the role of dust in astrophysical
processes. Chapter 2 discusses the cosmic history of the
chemical elements expected to be present in dust, and
examines the effect of gas-dust interactions on gas phase
abundances. Chapters 3-6 describe the observed properties
of interstellar grains, i.e., their extinction,
polarization, absorption and emission characteristics.
Chapters 7-9, discuss the origin and evolution of the dust,
tracing its life cycle in a succession of environments from
circumstellar shells to diffuse interstellar clouds,
molecular clouds, protostars and protoplanetary disks. The
final chapter summarizes progress toward a unified model.
Dust in other galaxies is discussed as an integral part of
the text rather than as a distinct topic requiring separate
chapters.
Containing extensive references and problems to aid
understanding and illustrate basic principles, the book is
ideally suited for graduate and advanced undergraduate
courses. It will also be an invaluable reference for
postgraduate students and researchers working in this
important field.
- Dust in the Galaxy: Our view from within.
- Abundances and depletions.
- Extinction and scattering.
- Polarization and grain alignment.
- Infrared absorption features.
- Continuum and line emission.
- Dust in stellar ejecta.
- Evolution of dust in the interstellar medium.
- The early phases of stellar evolution.
- Towards a unified model for interstellar dust.
- Appendices.
- References.
- Index
L'auteur - D C B Whittet
D C B Whittet, Rensselaer Polytechnic Institute, Troy,
New York, USA
Caractéristiques techniques
PAPIER | |
Éditeur(s) | Institute of Physics (IOP) |
Auteur(s) | D C B Whittet |
Parution | 07/02/2003 |
Édition | 2eme édition |
Nb. de pages | 390 |
Format | 15,5 x 23,5 |
Couverture | Broché |
Poids | 715g |
Intérieur | Noir et Blanc |
EAN13 | 9780750306249 |
ISBN13 | 978-0-7503-0624-9 |
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