Near Infrared Hydrogen Lines as Diagnostic of
Accretion and Winds in Young Stellar Objects



Hypertext version
Use it to browse through the thesis and see what it is all about.


Postscript files
If you decide you want to print it out.


Note: The quality of the plots in the postscript version is much better than in the hypertext version. You will note this, especially, in some plots of the earlier chapters.

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Daniel Folha

Last modified: Fri Sep 4 16:28:28 MET DST 1998