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CO observations,geometry, and galactic structure
Authors:B J Robinson  R N Manchester  W H McCutcheon
Institution:(1) Division of Radiophysics, CSIRO, Sydney, Australia;(2) University of British Columbia, Vancouver, Canada
Abstract:2.6 mm carbon monoxide and 21 cm hydrogen line observations of the Galaxy define six directions where gas is seen tangentially along a spiral feature and four directions where extended structures cross theR=R 0 circle. These directions provide a geometrical framework for any spiral structure pattern. Also simple equations are derived to define the normalized radiusR/R 0 of gas with a particular radial velocity in terms of the observed tangential velocity of gas with the sameR/R 0=sinl T, without specific knowledge of ohgr(R), ohgr0 orR 0.Paper presented at the IAU Third Asian-Pacific Regional Meeting, held in Kyoto, Japan, between 30 September–6 October, 1984.
Keywords:
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