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The discovery of the spiral arms of the Milky Way

Published online by Cambridge University Press:  04 August 2017

Owen Gingerich*
Affiliation:
Harvard-Smithsonian Center for Astrophysics

Abstract

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Attempts in the 1930s and 1940s to determine the spiral structure of the Milky Way by star counting methods, essentially the continuation of the work of the Kapteyn Astronomical Laboratory, failed to reach this goal. A new foundation for the search was laid by Walter Baade in his studies of stellar populations. With the recognition that highly luminous objects, especially H II regions, would outline the spiral structure, W.W. Morgan and his young associates Sharpless and Osterbrock carried out the observational program that first delineated, in 1951, the nearby arms of the Milky Way. The full paper was never published, so the historical details have remained somewhat vague, primarily because the 21-cm discoveries so quickly overtook the optical researches.

Type
PART I: HISTORY OF GALACTIC RESEARCH
Copyright
Copyright © Reidel 1985 

References

Notes and References

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11. Oral history interview with D.E. Osterbrock, on deposit at American Institute of Physics. I wish to thank Prof. Osterbrock for permission to quote from this interview and for his comments on the draft of this article. Photographs of the H II regions made with the Henyey-Greenstein camera are found in Sharpless, S. and Osterbrock, D., Astrophys. J. 115, pp. 8993, 1952.Google Scholar
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14. Morgan, W.W. to Gingerich, O., 25 March 1982.Google Scholar
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16. The Van Albada mentioned here is G.B. van Albada, later Director of the Lembang Observatory and of the Astronomical Institute at Amsterdam. (Editor.) Google Scholar