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Cosmical Gas Dynamics, Why Was It So Difficult?

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Kinematics and Dynamics of Diffuse Astrophysical Media

Abstract

When the invitation for this meeting reached me, I did not hesitate. Of course, I wished to be present when it was Franz Kahn’s turn for the formal move to say goodbye. Like many of us, he will probably sneak in again through the back door and continue working.

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References

I, II, III. See section 1 of this paper.

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Author information

Authors and Affiliations

  1. Sterrewacht, P.O.Box 9513, 2300, RA, Leiden, The Netherlands

    H. C. van de Hulst

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  1. H. C. van de Hulst
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Editor information

Editors and Affiliations

  1. The University, Manchester, England

    J. E. Dyson  & E. B. Carling  & 

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© 1994 Springer Science+Business Media Dordrecht

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van de Hulst, H.C. (1994). Cosmical Gas Dynamics, Why Was It So Difficult?. In: Dyson, J.E., Carling, E.B. (eds) Kinematics and Dynamics of Diffuse Astrophysical Media. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0926-0_1

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  • DOI: https://doi.org/10.1007/978-94-011-0926-0_1

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-4399-1

  • Online ISBN: 978-94-011-0926-0

  • eBook Packages: Springer Book Archive

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