Dynamics of Young Star Clusters and Associations Saas-Fee Advanced C
Where do most stars (and the planetary systems that surround them) in the Milky Way form? What determines whether a young star cluster remains bound (such as an open or globular cluster), or disperses to join the field stars in the disc of the Galaxy? The
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Cathie J. Clarke Robert D. Mathieu I. Neill Reid
Dynamics of Young Star Clusters and Associations
Saas-Fee Advanced Course 42
More information about this at http://www.springer.com/series/4284
Cathie J. Clarke Robert D. Mathieu I. Neill Reid •
Dynamics of Young Star Clusters and Associations Saas-Fee Advanced Course 42 Swiss Society for Astrophysics and Astronomy Edited by Cameron P.M. Bell, Laurent Eyer and Michael R. Meyer
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Volume Editors Cathie J. Clarke Institute for Astronomy University of Cambridge Cambridge UK
Cameron P.M. Bell Department of Physics and Astronomy University of Rochester Rochester, NY USA
Robert D. Mathieu Department of Astronomy University of Wisconsin Madison, WI USA
Laurent Eyer Department of Astronomy University of Geneva
I. Neill Reid Space Telescope Science Institute Baltimore, MD USA
Michael R. Meyer Institute for Astronomy ETH Zürich Zürich Switzerland
Sauverny Switzerland
This Series is edited on behalf of the Swiss Society for Astrophysics and Astronomy: Société Suisse d’Astrophysique et d’Astronomie Observatoire de Genève, ch. des Maillettes 51, CH-1290 Sauverny, Switzerland Cover illustration: The Orion Nebula Cluster, hosting several thousand stars and substellar objects, is the richest aggregate of young stars within 1500 light years (about 500 parsecs), and can be found within the ‘sword’ region of its eponymous constellation. CREDIT: NASA, ESA, M. Robberto (Space Telescope Science Institute/ESA) and the Hubble Space Telescope Orion Treasury Project Team. ISSN 1861-7980 Saas-Fee Advanced Course ISBN 978-3-662-47289-7 DOI 10.1007/978-3-662-47290-3
ISSN 1861-8227
(electronic)
ISBN 978-3-662-47290-3
(eBook)
Library of Congress Control Number: 2015946088 Springer Heidelberg New York Dordrecht London © Springer-Verlag Berlin Heidelberg 2015 This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed. The use of general descriptive names, registered names, trademarks, service marks, etc. in this publication does not imply, even in the absence of a specific statement, that such names are exempt from the relevant protective laws and regulations and therefore free for general use. The publisher, the authors and the editors are safe to assume that the advice and information in this book are believed to be true and accurate at the date of publication. Neither the publisher nor the authors or the editors give a warranty, express or implied, with respect to the material contained herein or for any errors or omissions that may have been made. Printed on acid-free paper Springer-Verlag GmbH Berlin Heidelberg is part of Springer Science+Business Media (www.springer.com)
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