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Novae and Related Stars

Proceedings of an International Conference Held by the Institut D’Astrophysique, Paris, France, 7 to 9 September 1976

  • M. Friedjung

Part of the Astrophysics and Space Science Library book series (ASSL, volume 65)

Table of contents

  1. Front Matter
    Pages I-XIV
  2. Novae, Dwarf Novae and Similar Objects at Minimum Light

  3. Observations of Novae and Related Objects During Outburst

  4. (a) Nebular Stage of Novae

  5. (b) Transient X Ray Sources

    1. Front Matter
      Pages 141-141
    2. F. Ciatti, A. Mammano, A. Vittone
      Pages 143-144
    3. C. Chevalier, E. Janot-Pacheco, H. Mauder, S. A. Ilovaisky
      Pages 145-145
    4. K. Pounds, M. Watson, C. Chevalier, S. A. Ilovaisky
      Pages 147-148
    5. S. A. Ilovaisky, C. Chevalier
      Pages 149-149
    6. H. W. Duerbeck
      Pages 150-150
  6. Observations of Nova Cygni 1975

    1. Front Matter
      Pages 153-153
    2. Yvette Andrillat
      Pages 155-176
    3. J. B. Hutchings
      Pages 178-178
    4. K. Kawara, T. Maihara, K. Noguchi, N. Oda, H. Okuda, S. Sato et al.
      Pages 179-179
    5. Irene Kupo, Elia M. Leibowitz
      Pages 180-180
    6. Waltraut Carola Seitter
      Pages 183-183
    7. Chi-Chao Wu
      Pages 184-184
    8. Sumner Starrfield, Warren M. Sparks, James W. Truran, J. S. Gallagher, P. A. Strittmatter, Hugh M. Van Horn
      Pages 185-185

About these proceedings

Introduction

Michael Friedjung Though known since antiquity, novae are still poorly under­ stood and present many problems. There has tended to be a lack of communication between theoreticians and observers and between different schools of thought, in spite of the advances of recent years in certain directions (observations of ordinary novae at minimum and of dwarf novae, theory of the causes of the explosion, etc ••• ). The meeting whose proceedings are contained in this volume was organized to stimulate a confron­ tation between the different ideas and results. The subject has changed a lot since 1963, when the previous international meeting was held. There were 61 participants at the conference from 17 countries, so very many groups ~oing research in the field of novae were represented. The reader will see that the subject has become more physical (we know for instance that the binary nature of novae is essential) but much work remains to be done. There is still a large gulf between theory and observation. May he find here many new ideas for future research! I would like to thank the French Centre National de la Recherche Scientifique for providing financial help. I must also thank the other members of the scientific committee (Profs and Drs Bath, Mustel, Payne-Gaposchkin, Sparks and Warner) and of the local committee (Audouze, Mrs Steinberg, Vauclair).

Keywords

Accretion LOPES accretion disk photometry spectroscopy stars stellar telescope

Editors and affiliations

  • M. Friedjung
    • 1
  1. 1.Institut d’AstrophysiqueParisFrance

Bibliographic information

  • DOI https://doi.org/10.1007/978-94-010-1217-1
  • Copyright Information Springer Science+Business Media B.V. 1977
  • Publisher Name Springer, Dordrecht
  • eBook Packages Springer Book Archive
  • Print ISBN 978-94-010-1219-5
  • Online ISBN 978-94-010-1217-1
  • Series Print ISSN 0067-0057
  • Buy this book on publisher's site
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