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Distribution of CO in the Southern Milky Way and large-scale structure in the Galaxy

Published online by Cambridge University Press:  04 August 2017

W.H. Mccutcheon ,
B. J. Robinson ,
R. N. Manchester  and
J. B. Whiteoak
W.H. Mccutcheon
Affiliation:
Department of Physics, University of British Columbia Vancouver, B.C.
B. J. Robinson
Affiliation:
Division of Radiophysics, CSIRO Sydney, Australia
R. N. Manchester
Affiliation:
Division of Radiophysics, CSIRO Sydney, Australia
J. B. Whiteoak
Affiliation:
Division of Radiophysics, CSIRO Sydney, Australia

Extract

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The southern galactic-plane region, in the ranges 294° ≤ 1 ≤ 358°, −0°.075 ≤ b ≤ 0°.075, has been surveyed in the J = 1–0 line of 12CO with a sampling interval of 3′ arc. Observations were made with the 4-metre telescope at the CSIRO Division of Radiophysics in 1980 and 1981. Details of equipment and observing procedure are given in Robinson et al. (1982, 1983); see also McCutcheon et al. (1983).

Information

Type
PART II: COMPOSITION, STRUCTURE AND KINEMATICS
Information
Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 203 - 204
Copyright
Copyright © Reidel 1985