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Planetary and Proto-Planetary Nebulae: From IRAS to ISO

Proceedings of the Frascati Workshop 1986, Vulcano Island, September 8–12, 1986

  • Andrea Preite Martinez

Part of the Astrophysics and Space Science Library book series (ASSL, volume 135)

Table of contents

  1. Front Matter
    Pages i-xi
  2. Session I

  3. Session II

  4. Session III

  5. Session IV

  6. Session V

  7. Session VI

    1. L. Rosino, T. Iijima, S. Ortolani, A. Mammano
      Pages 171-181
    2. R. Costero, M. Tapia, R. Méndez, J. Echevarría, M. Roth, A. Quintero et al.
      Pages 183-184
    3. M. de Muizon, A. Preite Martinez, M. Heydari-Malayeri
      Pages 185-196
    4. A. Preite Martinez, S. R. Pottasch
      Pages 197-202
    5. P. Persi, A. Preite Martinez, M. Ferrari-Toniolo, L. Spinoglio
      Pages 221-231
  8. Session VII

    1. P. Lenzuni, A. Natta, N. Panagia
      Pages 249-254
    2. A. Salama, P. De Bernardis, S. Masi, G. Moreno
      Pages 255-259
  9. Session VIII

    1. M. F. Kessler
      Pages 261-269
  10. Final Discussion

    1. Andrea Preite Martinez
      Pages 271-279
  11. Back Matter
    Pages 281-290

About these proceedings

Introduction

There are two questions that we can ask ourselves in order to describe this workshop. The first question is a double question: why a conference on this subject and why a workshop? The first idea of organizing this workshop came while reading the scientific objectives of one of the instruments onboard the ISO satel­ lite (a phase A document concerning the IR camera). On going through the scientific motivations for building the instrument I realized with surprise that no mention was made of Planetary Nebulae (PN). At present this is no longer true. There is a chapter indicating the capabilities of the camera in the PN field and what we can reasonably expect from that instrument. But it was at this moment that the first idea of organizing a workshop on the subject of PN came. Of course there are other, stronger motivations. The first one is that I think this is the right moment after IRAS. I think we all spent the last two or three years working on IRAS data. IRAS represented a corner-stone for those working on Planetary Nebulae: the amount of data that came out of the instruments onboard the satellite was enormous and opened up new ways of looking at planetary nebulae, as well as at other fields.

Keywords

astronomy observatory photometry planet spectroscopy star stars stellar

Authors and affiliations

  • Andrea Preite Martinez
    • 1
  1. 1.Istituto di Astrofisica SpazialeFrascatiItaly

Bibliographic information

  • DOI https://doi.org/10.1007/978-94-009-3891-5
  • Copyright Information Springer Science+Business Media B.V. 1987
  • Publisher Name Springer, Dordrecht
  • eBook Packages Springer Book Archive
  • Print ISBN 978-94-010-8228-0
  • Online ISBN 978-94-009-3891-5
  • Series Print ISSN 0067-0057
  • Buy this book on publisher's site
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