6. Mai 2013
ARI - Heidelberg
Europe/Berlin Zeitzone

Liste der Beiträge

1 von 1 angezeigt
  1. Dr. Richard Stancliffe (University of Bonn)
    A surprisingly large fraction of metal-poor stars are found to be carbon-rich. In addition, many of these display enhancements of neutron capture elements which give clues to their origin. I will discuss what we think we know about these so-called carbon-enhanced metal-poor (CEMP) stars, with a focus on those that display barium enrichments. These CEMP stars are thought to be formed in...
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