The following list summarizes the problems of and changes to the electronic version which was not implemented in the printed version - either because of the pagelimit or because the errors were found after the day of printing.
The list contains no minor changes (e.g. changed orders, added links, updated addresses etc.).

If you have problems with the electronic version, please read the technical information first; maybe its not a bug but a feature.
Please report any error to J.M.B. (via E-Mail: jbraun@astro.uni-bonn.de).

                                                             ;-) 

• There are some added sentences (marked by comments, i.e. visible in the HTML source) in the contribution "Recent Star Formation in the Wolf-Rayet BCDG MRK 1094", Méndez et al..
• The figures of the poster contribution "Interacting and merging processes between spirals and dwarf galaxies", Uwe Schwarzkopf and Ralf-Jürgen Dettmar, are only part of the electronic version.
• The second figure of the talk "The binary star cluster SL 538 / NGC 2006 (SL 537)", Andrea Dieball and Eva K. Grebel, is only part of the electronic version.
• The two figures (6 images) of the poster "Mass Segregation in Young LMC Clusters: NGC 2004 and NGC 2031", T. Richtler et al., are only included in the electronic version.
• Figure 3 of the talk "The Star Formation History of Nearby Dwarf Galaxies: problems, methods and results", Antonio Aparicio, is only part of the electronic version.
• A short description of "The Hubble Deep Field" project showing some images was added by J.M.B. to the electronic version.
• Netscape browsers have problems to display the entire review "Holes and Shells in Galaxies: Observations versus Theoretical Concepts", Jan Palous, so one has to click two times on reload to get the entire contribution [note the magic number '3'   8-)].
• ... the workshop got press release on 11th December 1998, so even trying to avoid further entries here, there will be some more in the future ...
• In Fig. 7b of the talk/poster contribution "The Young Large-Scale Features in the Large Magellanic Cloud", Jochen M. Braun, the scale length (500 pc) had been marked by a factor 1.4 too large.

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