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  3. The gas distribution in the central region of the Galaxy. III - A barlike model of the inner-Galaxy gas based on improved H I data
  1. Home
  2. Publications
  3. The gas distribution in the central region of the Galaxy. III - A barlike model of the inner-Galaxy gas based on improved H I data

The gas distribution in the central region of the Galaxy. III - A barlike model of the inner-Galaxy gas based on improved H I data

Authors:
  • HLH. S. Liszt
    H. S. Liszt
  • WBW. B. Burton
    W. B. Burton
Publisher website
Google Scholar
  • 1 March 1980
    • journal article
    • Published by American Astronomical Society in The Astrophysical Journal
    • Vol. 236, 779-797
    • DOI:10.1086/157803
Abstract
No abstract available
Keywords
  • ASTRONOMICAL MODELS
  • GALACTIC NUCLEI
  • GALACTIC STRUCTURE
  • GAS DENSITY
  • HYDROGEN CLOUDS
  • INTERSTELLAR GAS
  • MILKY WAY GALAXY
  • RADIO ASTRONOMY
  • ASTRONOMICAL MAPS
  • DISKS (SHAPES)
  • GAS DYNAMICS
  • HYDROGEN ATOMS
Cited by 180 articles
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