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New Views of Neutral Hydrogen in the Milky Way

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Book cover The Dense Interstellar Medium in Galaxies

Part of the book series: Springer Proceedings in Physics ((SPPHY,volume 91))

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Abstract

Since the first detection of neutral hydrogen (H i) by Ewen and Purcell in 1951 [4], H i has been a valuable tool for understanding the structure and dynamics of the Milky Way. The first analysis of H i in the Milky Way was also published in 1951 [14] and surveys of the entire Galaxy were immediately undertaken. In the intervening years the atlas of H i in the Milky Way has been continually updated, culminating most recently with the one arcminute resolution International Galactic Plane Survey.

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Author information

Authors and Affiliations

  1. Australia Telescope National Facility, CSIRO, 76, Epping, NSW, 1710, Australia

    N. M. McClure-Griffiths

Authors
  1. N. M. McClure-Griffiths
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Editor information

Editors and Affiliations

  1. Universität Köln I. Physikalisches Institut, Zülpicher Str. 77, 50937, Köln, Germany

    Susanne Pfalzner , Carsten Kramer  & Christian Straubmeier ,  & 

  2. Universität Bonn Radioastronomisches Institut, Auf dem Hügel 71, 53121, Bonn, Germany

    Andreas Heithausen

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© 1997 Springer-Verlag Berlin Heidelberg

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McClure-Griffiths, N.M. (1997). New Views of Neutral Hydrogen in the Milky Way. In: Pfalzner, S., Kramer, C., Straubmeier, C., Heithausen, A. (eds) The Dense Interstellar Medium in Galaxies. Springer Proceedings in Physics, vol 91. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-18902-9_35

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  • DOI: https://doi.org/10.1007/978-3-642-18902-9_35

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-642-62348-6

  • Online ISBN: 978-3-642-18902-9

  • eBook Packages: Springer Book Archive

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