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Table of contents

  1. Front Matter
  2. Steven M. Kahn, Duane A. Liedahl
    Pages 1-12
  3. R. Mewe
    Pages 13-25
  4. O. Vilhu, T. Tsum, A. Collier Cameron
    Pages 30-34
  5. J. S. Kaastra, J. A. M. Bleeker
    Pages 35-44
  6. W. A. Snyder, R. G. Cruddace, M. P. Kowalski, G. G. Fritz, E. E. Fenimore
    Pages 53-56
  7. Craig L. Sarazin, Michael W. Wise
    Pages 57-66
  8. M. P. Kowalski, W. A. Snyder, R. G. Cruddace, G. G. Fritz, E. O. Hulburt, E. E. Fenimore et al.
    Pages 72-75
  9. T. J. Ponman, M. P. Watt, P. A. Knight, D. Bertram, M. J. Church, C. J. Eyles et al.
    Pages 76-79
  10. T. R. Kallman
    Pages 85-97
  11. Yasuo Tanaka
    Pages 98-110
  12. Fumiaki Nagase
    Pages 111-121
  13. Monika Bałucińska-Church, Paul Barr
    Pages 130-133
  14. M. Gottwald, N.E. White
    Pages 134-137
  15. B. J. Kellett, E. N. Ercan, A. M. Cruise
    Pages 143-146
  16. W. Brinkmann, N. Kawai, M. Matsuoka
    Pages 147-150
  17. E. V. Seifina, N. I. Shakura, K. A. Postnov, M. E. Prokhorov
    Pages 151-154
  18. A. J. Norton, M. G. Watson, A. R. King
    Pages 155-161
  19. A. C. Fabian, I. M. George
    Pages 167-176
  20. K. Nandra, K. A. Pounds, G. C. Stewart
    Pages 177-186
  21. I. M. George, A. C. Fabian, R. R. Ross
    Pages 196-200
  22. G. Matt, G. C. Perola, L. Piro
    Pages 201-204
  23. J. Felsteiner, R. Opher
    Pages 209-213
  24. Gabriele Ghisellini, Andrzej A. Zdziarski, Ian M. George, Roland Svensson, A. C. Fabian, Chris Done
    Pages 214-217
  25. Bożena Czerny, Magda Zbyszewska, D. J. Raine
    Pages 226-229
  26. H. Kunieda, H. Awaki, K. Koyama, Y. Tawara, Y. Tsusaka, C. Done et al.
    Pages 241-246
  27. F. Fiore, G. C. Perola, L. Piro, M. Yamauchi, M. Matsuoka
    Pages 251-254
  28. G. C. Perola
    Pages 259-266
  29. Herbert W. Schnopper
    Pages 274-283
  30. N. J. Westergaard, H. U. Nørgaard-Nielsen, F. E. Christensen, A. Hornstrup, C. Budtz-Jørgensen, B. Byrnak et al.
    Pages 284-288
  31. Stephen S. Holt
    Pages 289-299
  32. G. Shaviv, T. Weller, J. Felsteiner, B. Rosner, M. Livio, N. Lupu et al.
    Pages 311-319
  33. Back Matter

About these proceedings

Introduction

Transitions from the innermost shells of iron, especially the K- and L-shelllines, provide a powerful tool for probing the physical characteristics of hot plasmas in X-ray sources. Their strength and purity allow important conclusions to be drawn even with modest energy resolution. They should also help in studying the regions around black holes and neutron stars. In this book the state of the art and themost recent theoretical and experimental observations are presented. The book will be a valuable source for future satellite missions. It addresses both researchers and graduate students in astrophysics.

Keywords

Astrophysik Plasma Röntgenspektroskopie X-ray spectroscopy astrophysics plasma physics spectroscopy

Bibliographic information

  • DOI https://doi.org/10.1007/BFb0031264
  • Copyright Information Springer-Verlag 1991
  • Publisher Name Springer, Berlin, Heidelberg
  • eBook Packages Springer Book Archive
  • Print ISBN 978-3-540-54354-1
  • Online ISBN 978-3-540-47583-5
  • Series Print ISSN 0075-8450
  • Series Online ISSN 1616-6361
  • Buy this book on publisher's site
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