Millimeter Astronomy Saas-Fee Advanced Course 38. Swiss Society for
The millimeter and sub-millimeter wavebands are unique in astronomy in containing several thousands of spectral lines of molecules as well as the thermal continuum spectrum of cold dust. They are the only bands in the electromagnetic spectrum in which we
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T. L. Wilson Stéphane Guilloteau
Millimeter Astronomy
Saas-Fee Advanced Course 38
More information about this series at http://www.springer.com/series/4284
T. L. Wilson Stéphane Guilloteau •
Millimeter Astronomy Saas-Fee Advanced Course 38 Swiss Society for Astrophysics and Astronomy Edited by Miroslava Dessauges-Zavadsky and Daniel Pfenniger
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Authors T. L. Wilson Max-Planck-Institut für Radioastronomie Bonn Germany Stéphane Guilloteau Laboratoire d’Astrophysique de Bordeaux Université Bordeaux 1 Bordeaux France
Volume Editors Miroslava Dessauges-Zavadsky Observatoire de Genève Université de Genève Sauverny Switzerland Daniel Pfenniger Observatoire de Genève Université de Genève 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: A montage of ALMA Antennae, Credit ESO, with Barnard 150 Dark Nebula in Cepheus, http://www.astrogb.com/b150.htm, © Giovanni Benintende, Reproduced with permission
ISSN 1861-7980 ISSN 1861-8227 (electronic) Saas-Fee Advanced Course ISBN 978-3-662-57545-1 ISBN 978-3-662-57546-8 (eBook) https://doi.org/10.1007/978-3-662-57546-8 Library of Congress Control Number: 2018943384 © Springer-Verlag GmbH Germany, part of Springer Nature 2018 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. The publisher remains neutral with regard to jurisdictional claims in published maps and institutional affiliations. Printed on acid-free paper This Springer imprint is published by the registered company Springer-Verlag GmbH, DE part of Springer Nature The registered company address is: Heidelberger Platz 3, 14197 Berlin, Germany
Preface
The millimeter (mm) and sub-millimeter (sub-mm) wavebands are unique in astronomy in containing more than 1000 spectral lines of molecules as well as the thermal continuum spectrum of cold dust. They are the only bands in the el
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