CO observations,geometry, and galactic structure |
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Authors: | B J Robinson R N Manchester W H McCutcheon |
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Institution: | (1) Division of Radiophysics, CSIRO, Sydney, Australia;(2) University of British Columbia, Vancouver, Canada |
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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 (R), 0 orR
0.Paper presented at the IAU Third Asian-Pacific Regional Meeting, held in Kyoto, Japan, between 30 September–6 October, 1984. |
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Keywords: | |
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