The puzzling frequencies of CEMP and NEMP stars

Abstract

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

Similar works

Full text

thumbnail-image

Utrecht University Repository

redirect
Last time updated on 14/06/2016

This paper was published in Utrecht University Repository.

Having an issue?

Is data on this page outdated, violates copyrights or anything else? Report the problem now and we will take corresponding actions after reviewing your request.