Skip to main content
Article thumbnail
Location of Repository

The puzzling frequencies of CEMP and NEMP stars

By O.R. Pols, R.G. Izzard, E. Glebbeek and R.J. Stancliffe


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 modifications of the initial mass function at low metallicity

Year: 2009
OAI identifier:
Download PDF:
Sorry, we are unable to provide the full text but you may find it at the following location(s):
  • (external link)
  • Suggested articles

    To submit an update or takedown request for this paper, please submit an Update/Correction/Removal Request.