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4. Conclusions

In conclusion, the velocities presented here give a significant improvement over older data for planetary nebulae in the Galactic bulge. The majority of these nebulae in the direction of the Bulge have estimated distances and velocities consistent with bulge membership.


We are grateful to Bjorn Stenholm who participated in some of the observations, and to Dante Minniti who gave helpful comments.

Copyright by the European Southern Observatory (ESO)