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Distribution of CO in the Southern Milky Way

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Kinematics, Dynamics and Structure of the Milky Way

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 100))

Abstract

A survey of J = 1−0 12CO emission in the ranges 294° ≤ ℓ ≤ 358°, −0°.075 ≤ b ≤ 0°.075 has been made with observations spaced at 3’ arc intervals. Results pertaining to the large-scale properties of the Galaxy are presented.

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Author information

Authors and Affiliations

  1. Department of Physics, University of British Columbia, Vancouver, B.C., Canada

    W. H. McCutcheon

  2. Division of Radiophysics, CSIRO, Sydney, Australia

    B. J. Robinson, J. B. Whiteoak & R. N. Manchester

Authors
  1. W. H. McCutcheon
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  2. B. J. Robinson
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  3. J. B. Whiteoak
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  4. R. N. Manchester
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Editor information

Editors and Affiliations

  1. Department of Physics, University of British Columbia, Vancouver, B.C., V6T 1W5, Canada

    W. L. H. Shuter

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© 1983 D. Reidel Publishing Company, Dordrecht, Holland

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McCutcheon, W.H., Robinson, B.J., Whiteoak, J.B., Manchester, R.N. (1983). Distribution of CO in the Southern Milky Way. In: Shuter, W.L.H. (eds) Kinematics, Dynamics and Structure of the Milky Way. Astrophysics and Space Science Library, vol 100. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7060-1_26

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  • DOI: https://doi.org/10.1007/978-94-009-7060-1_26

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-009-7062-5

  • Online ISBN: 978-94-009-7060-1

  • eBook Packages: Springer Book Archive

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