Kinematics and Dynamics of Diffuse Astrophysical Media

  • J. E. Dyson
  • E. B. Carling

Table of contents

  1. Front Matter
    Pages i-xii
  2. H. C. van de Hulst
    Pages 1-12
  3. Bruce Balick
    Pages 13-22
  4. M. Bryce, J. Meaburn, B. Balick, J. R. Walsh
    Pages 23-24
  5. L. Cuesta, J. P. Phillips, A. Mampaso
    Pages 25-29
  6. S. M. Scarrott, R. M. J. Scarrott, R. D. Wolstencroft
    Pages 31-42
  7. A. Riera, P. García-Lario, A. Manchado
    Pages 43-44
  8. A. F. J. Moffat, S. Lépine, R. N. Henriksen, C. Robert
    Pages 55-65
  9. T. P. Ray
    Pages 71-86
  10. L. M. Chernin, C. R. Masson
    Pages 113-117
  11. S. A. E. G. Falle
    Pages 119-125
  12. S. Biro, A. C. Raga
    Pages 127-128
  13. Rachael Padman, John S. Richer
    Pages 129-134
  14. Jochen Eislöffel
    Pages 135-136
  15. S. Curiel, J. M. Moran, L. F. Rodríguez, J. Cantó
    Pages 137-138
  16. J. J. Wiseman, P. T. P. Ho
    Pages 139-142
  17. M. T. Malone, J. E. Dyson, T. W. Hartquist
    Pages 143-150
  18. R. López, O. Morata, I. Sepúlveda, R. Estalella, G. Anglada, J. Pastor et al.
    Pages 151-152
  19. S. D. Taylor, D. A. Williams, T. W. Hartquist
    Pages 153-154
  20. J. M. C. Rawlings, N. J. Evans II, S. Zhou
    Pages 155-157
  21. M. P. Hobson
    Pages 159-160
  22. H. M. Lloyd, T. J. O’Brien, M. F. Bode, F. D. Kahn
    Pages 161-166
  23. T. J. O’Brien, H. M. Lloyd
    Pages 167-172
  24. L. Woltjer, M. P. Véron-Cetty
    Pages 173-177
  25. T. W. Hartquist
    Pages 185-200
  26. J. J. Quenby, T. J. Sumner, S. D. Sidher, S. Immler
    Pages 213-217
  27. T. W. Hartquist, G. E. Morfill
    Pages 223-234
  28. J. A. Turner, A. P. Whitworth
    Pages 239-240
  29. You-Hua Chu, Robert C. Kennicutt Jr.
    Pages 253-262
  30. J. Meaburn, R. M. Massey
    Pages 263-265
  31. J. Meaburn, J. E. Dyson, C. D. Goudis, P. E. Christopoulou
    Pages 281-283
  32. Héctor O. Castañeda
    Pages 285-289
  33. D. Breitschwerdt, F. D. Kahn
    Pages 297-301
  34. J. C. Raymond, S. Curiel
    Pages 303-309

About this book


The area of diffuse astrophysical media is enormous and ranges over circum­ stellar to extragalactic scales. The physical conditions can vary from cool dusty gases to collections of relativistic particles. Flows in such media are set up by en­ ergy and momentum injection from winds, jets and explosions. The study of these phenomena involves physics, chemistry and, inevitably, hydrodynamics. One of the most important aspects of this study is the ever increasing overlap between theory and observation. Indeed, it can be argued that the only way to really understand these complex flows which can never be duplicated under terrestrial conditions, is to encourage this overlap, and this was one major aim of this Conference. Because of the long theoretical and observational association of the Manchester Group with this general area, Manchester seemed an appropriate venue for this Con­ ference. But in fact this long association and the actual year of the Conference are connected. In 1951 Franz Kahn joined the Astronomy Department at Manchester University and immediately the study of diffuse media, particularly the hydrody­ namic aspects, commenced and has flourished ever since. Franz became Head of the Astronomy Department in 1981 following the retirement of Professor Z. Kopal, who founded the Department and was instrumental in attracting Franz to it. In 1993, Franz retired from this position and a most serendipidous coincidence was his election to the Royal Society announced shortly before the Conference.


LOPES Population Variation active galactic nuclei cosmic ray galaxy gravitation magnetosphere nebula planet relativistic jet star star formation stellar turbulence

Editors and affiliations

  • J. E. Dyson
    • 1
  • E. B. Carling
    • 1
  1. 1.The UniversityManchesterEngland

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