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AbstractAbstract
[en] The authors have significantly extended the observations of CO emission from molecular clouds in a number of ways: (1) they have extended longitude coverage, and now have at least some data taken over the range 45 deg < l < 230 deg (with no data taken within 20 deg of the anticenter); (2) they have extended latitude coverage to enable to estimate the location of the midplane and the thickness of the CO emitting layer; (3) they have greatly extended the mapping, now having at least partial CO maps of 55 clouds, along with 13CO, C18O, CO(2 → 1), and 2-mm H2CO observations of some clouds. (Auth.)
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Burton, W.B.; Israel, F.P. (eds.); Astrophysics and Space Science Library; v. 105; 309 p; ISBN 90-277-1651-X;
; 1983; p. 143-148; D. Reidel; Dordrecht (Netherlands); Workshop on surveys of the Southern Galaxy; Leyden (Netherlands); 4-6 Aug 1982; 4 figs.

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Conference
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