High-resolution X-ray plasma diagnostics of stellar coronae

Dissertation zur Erlangung des Doktorgrades des Fachbereichs Physik der Universität Hamburg

vorgelegt von Jan-Uwe Ness aus Oldenburg

Hamburg, 2002

Gutachter der Dissertation: Prof. Dr. J. H. M. M. Schmitt
Prof. Dr. D. Reimers
Gutachter der Disputation: Prof. Dr. J. H. M. M. Schmitt
Prof. Dr. H. J. Wendker
Tag der Disputation: 05.3.2002
Dekan des Fachbereichs
Physik und Vorsitzender
des Promotionsausschusses: Prof. Dr. F.-W. Büßer

Contents (Postscript, 205 kB)
Abstract
Zusammenfassung
Conclusions
Danksagung/Acknowledgments
1. Introduction (Postscript, 16MB)
HTML
2. Cora line fitting tool (Postscript, 540 kB)
3. Density diagnostics for Capella and Procyon (Postscript, 2.6 MB)
4. Analysis of a Chandra LETGS spectrum of Algol (Postscript, 3.4 MB)
5. Coronal density diagnostics for seven cool stars (Postscript, 1.7 MB)
6. Influence of UV radiation fields on the density diagnostics for Algol and Procyon (Postscript, 4.0 MB)
7. Influence of UV radiation fields on density diagnostics with He-like triplets (Postscript, 4.1 MB)
8. Summary and concluding remarks (Postscript, 265 kB)
9. List of Publications (Postscript, 791 kB)
Lebenslauf (Postscript, 45 kB)

Complete thesis (gziped Postscript, 7.6 MB) (PDF, 7.9 MB)