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Toward a New Millennium in Galaxy Morphology pp 59–78Cite as

Neutral Hydrogen and Dark Matter in Spiral Galaxies

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Abstract

The first part presents a brief review of the main HI properties of isolated, normal spiral galaxies and of the phenomena which seem to characterize and dominate their internal metabolism. In the second part attention is drawn to all those processes, such as tidal interactions, accretion and mergers, that depend on the galaxy environment and may play a significant role in galaxy formation and evolution. In the third part the observational evidence for the dark matter component of spiral galaxies is discussed.

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Authors and Affiliations

  1. Osservatorio Astronomico di Bologna, Via Ranzani 1, 1-40127, Bologna, Italy

    Renzo Sancisi

  2. Kapteyn Astronomical Institute, PO Box 800, 9700, AV, Groningen, The Netherlands

    Renzo Sancisi

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  1. Renzo Sancisi
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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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Sancisi, R. (2000). Neutral Hydrogen and Dark Matter in Spiral 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_4

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  • DOI: https://doi.org/10.1007/978-94-011-4114-7_4

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