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A Mid and Far Infrared View of Galaxies

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Toward a New Millennium in Galaxy Morphology

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Abstract

From the disk of normal galaxies to the nucleus of prototype active sources, we review the wealth of results and new understanding provided by recent infrared probes and, in particular, the four instruments on-board of ISO.

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Author information

Authors and Affiliations

  1. C.E.A. Saclay, DSM/DAPNIA/Service d’Astrophysique, 91191, Gif sur Yvette Cedex, France

    C. J. Cesarsky

  2. European Southern Observatory, Karl-Schwarzschildstr. 2, D-85754, Garching bei München, Germany

    C. J. Cesarsky

  3. C.E.A. Saclay, DSM/DAPNIA/Service d’Astrophysique, 91191, Gif sur Yvette Cedex, France

    M. Sauvage

Authors
  1. C. J. Cesarsky
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  2. M. Sauvage
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Editor information

Editors and Affiliations

  1. Department of Computational and Applied Mathematics, University of the Witwatersrand, Johannesburg, South Africa

    David L. Block

  2. Optica y Electrónica, Instituto Nacional de Astrofísica, Calle Luis Enrique Erro I, Tonantzintla, Puebla, México

    Ivânio Puerari

  3. Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, Hawaii, USA

    Alan Stockton

  4. Delia Park 32, Delia Street, Dorandia, Pretoria, South Africa

    Dewet Ferreira

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Cesarsky, C.J., Sauvage, M. (2000). A Mid and Far Infrared View of Galaxies. In: Block, D.L., Puerari, I., Stockton, A., Ferreira, D. (eds) Toward a New Millennium in Galaxy Morphology. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4114-7_22

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  • DOI: https://doi.org/10.1007/978-94-011-4114-7_22

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