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Infrared Astronomy

Proceedings of the NATO Advanced Study Institute held at Erice, Sicily, 9–20 July, 1977

  • Conference proceedings
  • © 1978

Overview

Part of the book series: Nato Science Series C: (ASIC, volume 38)

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Table of contents (16 papers)

  1. Interstellar Matter

  2. Infrared Observations of HII Regions

  3. Physics and Astrophysics of Interstellar Dust

  4. Physics of Molecular Clouds from Millimeter Wave Line Observations

  5. Theoretical Aspects of the Infrared Emission from HII Regions

  6. Star Formation and Related Topics

  7. Infrared Emission of the Galactic Center and Extragalactic Sources

  8. Infrared Astronomical Background Radiation

  9. Cosmic Background: Measurements of the Spectrum

  10. Cosmological Aspects of Infrared and Millimetre Astronomy

  11. Observational Techniques in Infrared Astronomy

  12. Infrared Astronomical Spectroscopy

  13. Infrared Astronomy from Space: A Review of Future Possibilities

  14. Seminars

Keywords

About this book

This volume contains a series of lectures presented at the 4th Course of the International School of Astrophysics, held in Erice (Sicily) from July 9 - July 20, 1977 at the "E. Majorana" Centre for Scientific Culture. The course was fully supported by a grant from the NATO Advanced Study Institute Programme. It was attended by 82 participants from 15 countries. Even though the infrared portion of the electromagnetic spectrum covers an extensive interval from the red region of the optical spectrum (10,000 A) to the microwave radio region (1 mm), its role in astronomy has been minimal until the last two decades. Until very recently, the only objects observed were the sun, the moon and the planets. A primary reason for this late development was the lack of sensitive detectors and the necessary cryogenic technology that must accompany their use. Recent progress in this technology has been paralleled by an ever increasing interest of astronomers in infrared observations, leading to a number of ex­ tremely important results in different branches of astronomy. This becomes evident when one realizes that in many astrophysical conditions most of the energy is found to be channeled into the infrared portion of the electromagnetic spectrum. Stars were detected that yield most of their radiation in the infrared; these objects present a new view of stellar evolution, both in the birth and death stages.

Editors and Affiliations

  • Laboratorio di Radioastronomia CNR, University of Bologna, Italy

    Giancarlo Setti

  • Harvard-Smithsonian Center for Astrophysics, Cambridge, USA

    Giovanni G. Fazio

Bibliographic Information

  • Book Title: Infrared Astronomy

  • Book Subtitle: Proceedings of the NATO Advanced Study Institute held at Erice, Sicily, 9–20 July, 1977

  • Editors: Giancarlo Setti, Giovanni G. Fazio

  • Series Title: Nato Science Series C:

  • DOI: https://doi.org/10.1007/978-94-009-9815-5

  • Publisher: Springer Dordrecht

  • eBook Packages: Springer Book Archive

  • Copyright Information: D. Reidel Publishing Company, Dordrecht, Holland 1978

  • Hardcover ISBN: 978-90-277-0871-7Due: 31 December 1978

  • Softcover ISBN: 978-94-009-9817-9Published: 20 November 2011

  • eBook ISBN: 978-94-009-9815-5Published: 06 December 2012

  • Series ISSN: 1389-2185

  • Edition Number: 1

  • Number of Pages: 368

  • Topics: Astronomy, Observations and Techniques

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