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Wolf-Rayet stars, ring-type H II regions, and spiral structure

Published online by Cambridge University Press:  14 August 2015

Th. Schmidt-Kaler
Th. Schmidt-Kaler*
Affiliation:
Astronomisches Institut, Ruhr-Universität, Bochum, Germany

Extract

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At the Prague IAU meeting (Isserstedt and Schmidt-Kaler, 1967) we presented some results of investigations on stellar rings, a new kind of stellar association and powerful spiral tracer. We have since kept looking for similar features of gas or dust which might be early stages in the evolution of stellar rings.

Type
Part II/Observations of Spiral Structure in Our Galaxy
Information
Symposium - International Astronomical Union , Volume 38: The Spiral Structure of our Galaxy , 1970 , pp. 284 - 286
Copyright
Copyright © Reidel 1970 

References

Becker, W. and Fenkart, R. P.: 1970, IAU Symposium No. 38, p. 205.CrossRefGoogle Scholar
Freeman, K. C., Rodgers, A. W., and Lyngå, G.: 1968, Nature 219, 251.CrossRefGoogle Scholar
Hiltner, W. A. and Schild, R. E.: 1966, Astrophys. J. 143, 770.CrossRefGoogle Scholar
Isserstedt, J.: 1970, IAU Symposium No. 38, p. 287.CrossRefGoogle Scholar
Isserstedt, J. and Schmidt-Kaler, T.: 1967, Preprint, see also Sky Telesc. 34, 299.Google Scholar
Schmidt-Kaler, T.: 1968, Veröff. Bochum No. 1, 80.CrossRefGoogle Scholar
Schmidt-Kaler, T.: 1969, Colloque Internat. Liège, No. 16.Google Scholar
Smith, L. F.: 1968, Monthly Notices Roy. Astron. Soc. 141, 317.CrossRefGoogle Scholar
Westphal, J. A., Sandage, A., and Kristian, J.: 1968, Astrophys. J. 154, 139.CrossRefGoogle Scholar