Modelling the fraction of Lyman break galaxies with strong Lyman α emission at 5 ≤ z ≤ 7

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©:2011 RAS © 2011 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

Detalhes bibliográficos
Autores: Forero-Romero, Jaime E., Yepes Alonso, Gustavo, Gottlöber, Stefan, Prada, Francisco
Tipo de documento: artigo
Data de publicação:2012
País:España
Recursos:Universidad Autónoma de Madrid
Repositório:Biblos-e Archivo. Repositorio Institucional de la UAM
Idioma:inglês
OAI Identifier:oai:repositorio.uam.es:10486/666884
Acesso em linha:http://hdl.handle.net/10486/666884
https://dx.doi.org/10.1111/j.1365-2966.2011.19744.x
Access Level:Acceso aberto
Palavra-chave:Galaxies: evolution
Galaxies: high-redshift
Física
Descrição
Resumo:This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©:2011 RAS © 2011 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.