The carbon-enhanced metal-poor (CEMP) stars constitute approximately one fifth of the metal-poor ([Fe/H
We present a detailed study of carbon-enhanced metal-poor (CEMP) stars, based on high-resolution spe...
We present a comprehensive abundance analysis of two newly discovered carbon-enhanced metal-poor (CE...
The stellar population in the Galactic halo is characterised by a large fraction of carbon-enhanced ...
The carbon-enhanced metal-poor (CEMP) stars constitute approximately one fifth of the metal-poor ([F...
Abstract: We construct binary-star population nucleosynthesis models of carbon-enhanced metal poor (...
The carbon-enhanced metal-poor (CEMP) stars constitute approximately one fifth of the metal-poor ($[...
We present the results of binary population simulations of carbon-enhanced metal-poor (CEMP) stars. ...
Context. An increasing fraction of carbon-enhanced metal-poor (CEMP) stars is found as their iron ab...
9Context. An increasing fraction of carbon-enhanced metal-poor (CEMP) stars is found as their iron...
Recent spectroscopic surveys have revealed a large number of extremely metal-poor stars in the Galac...
International audienceAims. Carbon-enhanced metal-poor (CEMP) stars represent a sizeable fraction of...
A new class of carbon-rich stars was revealed by large surveys of very metal-poor objects, the carbo...
Most carbon-enhanced metal-poor (CEMP) stars are thought to result from past mass transfer of He-bur...
Contains fulltext : 147328.pdf (preprint version ) (Open Access
Many of the carbon-enhanced metal-poor (CEMP) stars that we observe in the Galactic halo are found i...
We present a detailed study of carbon-enhanced metal-poor (CEMP) stars, based on high-resolution spe...
We present a comprehensive abundance analysis of two newly discovered carbon-enhanced metal-poor (CE...
The stellar population in the Galactic halo is characterised by a large fraction of carbon-enhanced ...
The carbon-enhanced metal-poor (CEMP) stars constitute approximately one fifth of the metal-poor ([F...
Abstract: We construct binary-star population nucleosynthesis models of carbon-enhanced metal poor (...
The carbon-enhanced metal-poor (CEMP) stars constitute approximately one fifth of the metal-poor ($[...
We present the results of binary population simulations of carbon-enhanced metal-poor (CEMP) stars. ...
Context. An increasing fraction of carbon-enhanced metal-poor (CEMP) stars is found as their iron ab...
9Context. An increasing fraction of carbon-enhanced metal-poor (CEMP) stars is found as their iron...
Recent spectroscopic surveys have revealed a large number of extremely metal-poor stars in the Galac...
International audienceAims. Carbon-enhanced metal-poor (CEMP) stars represent a sizeable fraction of...
A new class of carbon-rich stars was revealed by large surveys of very metal-poor objects, the carbo...
Most carbon-enhanced metal-poor (CEMP) stars are thought to result from past mass transfer of He-bur...
Contains fulltext : 147328.pdf (preprint version ) (Open Access
Many of the carbon-enhanced metal-poor (CEMP) stars that we observe in the Galactic halo are found i...
We present a detailed study of carbon-enhanced metal-poor (CEMP) stars, based on high-resolution spe...
We present a comprehensive abundance analysis of two newly discovered carbon-enhanced metal-poor (CE...
The stellar population in the Galactic halo is characterised by a large fraction of carbon-enhanced ...