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Compression of interstellar clouds in spiral density-wave shocks

Published online by Cambridge University Press:  14 August 2015

Paul R. Woodward
Paul R. Woodward*
Affiliation:
Leiden Observatory, The Netherlands, and Lawrence Livermore Laboratory, Livermore, Calif.

Abstract

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A mechanism of triggering star formation by galactic shocks is discussed.

Type
III. SPIRAL STRUCTURE
Information
Symposium - International Astronomical Union , Volume 84: The Large-Scale Characteristics of the Galaxy , 1979 , pp. 159 - 164
Copyright
Copyright © Reidel 1979 

References

Elmegreen, B. G., and Lada, C. J. 1977. Ap. J. 214, pp. 725–41.Google Scholar
Gerwin, R. A. 1968. Rev. Mod. Phys. 40, pp. 652–8.Google Scholar
Herbst, W., and Assousa, G. E. 1977. Ap. J. 217, pp. 473–87.Google Scholar
Noh, W. F., and Woodward, P. R. 1976. Proc. Int. Conf. Numer. Methods Fluid Dyn., 5th, Enschede, Netherlands, 1976, pp. 330–40.Google Scholar
Roberts, W. W. 1969. Ap. J. 158, pp. 123–43.Google Scholar
Sutcliffe, W. G. 1973. Tech. Rpt. UCID-17013, Lawrence Livermore Lab, Livermore, Calif.Google Scholar
Woodward, P. R. 1976. Ap. J. 207, pp. 484–501.Google Scholar