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Radial velocities as a guide to spiral structure

Published online by Cambridge University Press:  14 August 2015

A. D. Thackeray
A. D. Thackeray*
Affiliation:
Radcliffe Observatory

Extract

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Four main methods of delineating spiral structure in the Galaxy have been developed in the past 10 years.

Type
Section 1: The Galaxy
Information
Symposium - International Astronomical Union , Volume 20: The Galaxy and the Magellanic Clouds , 1964 , pp. 155 - 158
Copyright
Copyright © Australian Academy of Science 1964 

References

Kerr, F. J. (1962).— M.N. 123: 327–45.Google Scholar
Münch, G. (1957).— Ap. J. 125: 42–65.CrossRefGoogle Scholar
Thackeray, A. D. (1956).— Nature 178: 1458.CrossRefGoogle Scholar