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Abstract submission - closed as of June 15
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Splinter Sessions

Use this listing as source of information and to give feedback to the conveners. Refer to the (to be published) final program to find out when your favorite splinter session has been scheduled.

Disclaimer: These summaries are generated almost fully automatically from the submissions.

To the conveners: If you want to update the applications (esp. in case you got feedback about more participants), contact me at aschweitzer@hs.uni-hamburg.de.

• Formation and Evolution of very Low Mass Stars and Brown Dwarfs
• Magnetic Activity in young stars
• The relevance and future of the Ultraviolet Range
• Spectral Classification beyond M
• What future for stellar X-ray Spectroscopy ?
• Mass-loss across the Giant Branches
• Imaging of Cool Stars

This document was translated from L^AT_EX by H^EV^EA and H^AC^HA.

Last modified: Tuesday, 01-Jun-2004 15:14:59 CEST | Comments or problems to A. Schweitzer