Journal
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA
Volume 26, Issue 3, Pages 327-329Publisher
CSIRO PUBLISHING
DOI: 10.1071/AS08076
Keywords
stars: AGB and post-AGB; stars: abundances; stars: binaries; stars: evolution; stars: mass function
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Funding
- NWO [614.000.424]
- Australian Research Council's [DP0879472]
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We present the results of binary population simulations of carbon- and nitrogen-enhanced metal-poor (CEMP and NEMP) stars. We show that the observed paucity of very nitrogen-rich stars puts strong constraints on possible modi. cations of the initial mass function at low metallicity.
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