Chemical Evolution of Dwarf Galaxies and Stellar Clusters: Conference Summary

Details Chemical Evolution of Dwarf Galaxies and Stellar Clusters: Conference Summary Chemical Evolution of Dwarf Galaxies and Stellar Clusters: Conference Summary

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008msngr.134s..28f&link_type=abstract

The Messenger, vol. 134 supplement, p. 28-30

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The summary begins by considering the contributions on the differences between globular clusters (GCs) and dwarf spheroidal (dSph) galaxies. Then I discuss globular clusters: the topics include multiple sequences in the colour-magnitude plane, light element abundance anomalies, globular cluster systems and other issues. The next section is devoted to dwarf galaxies, summarising new results on their kinematics, masses and baryon content, their star formation histories, and their chemical abundance ranges and chemical signatures. The last section discusses some of the other interesting related points that came up during the meeting.

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