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

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Postscript files

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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.

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